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searching for Low Mass 487 found (1735 total)

alternate case: low Mass

Stellar mass (1,213 words) [view diff] no match in snippet view article find links to article

behavior as they approach the end of their nuclear fusion lifetimes. Very-low-mass stars with masses below 0.5 M☉ do not enter the asymptotic giant branch

X-ray binary (1,706 words) [view diff] no match in snippet view article find links to article

separation. An estimated 1041 positrons escape per second from a typical low-mass X-ray binary. X-ray binaries are further subdivided into several (sometimes

Exoplanet orbital and physical parameters (6,472 words) [view diff] no match in snippet view article find links to article

surprising, because current theories of planetary formation suggest that low-mass planets should have their orbital eccentricity circularized by gravitational

Helium flash (1,615 words) [view diff] no match in snippet view article find links to article

of helium into carbon through the triple-alpha process in the core of low-mass stars (between 0.8 solar masses (M☉) and 2.0 M☉) during their red giant

Lithium burning (511 words) [view diff] no match in snippet view article find links to article

a star. Lithium is generally present in brown dwarfs and not in older low-mass stars. Stars, which by definition must achieve the high temperature (2

Star formation (5,539 words) [view diff] no match in snippet view article find links to article

outflows.[jargon] Observations indicate that the coldest clouds tend to form low-mass stars, which are first observed via the infrared light they emit inside

Brown dwarf (20,254 words) [view diff] case mismatch in snippet view article find links to article

(possibly a low-mass star) or a young brown dwarf with a very low mass. For Y dwarfs this is less of a problem, as they remain low-mass objects near

Gas giant (1,908 words) [view diff] no match in snippet view article find links to article

by the Grand tack hypothesis. The defining differences between a very low-mass brown dwarf (which can have a mass as low as roughly 13 times that of Jupiter)

Red dwarf (4,244 words) [view diff] no match in snippet view article find links to article

avoiding helium buildup at the core, thereby prolonging the period of fusion. Low-mass red dwarfs therefore develop very slowly, maintaining a constant luminosity

Stellar evolution (6,476 words) [view diff] no match in snippet view article find links to article

become brighter and hotter before running out of hydrogen fuel and becoming low-mass white dwarfs. Stellar evolution is not studied by observing the life of

3XMM J004232.1+411314 (603 words) [view diff] no match in snippet view article find links to article

3XMM J004232.1+411314 is a low-mass X-ray binary hosted in the galaxy M31. It is the most luminous source of hard X-rays in the Andromeda Galaxy. It is

Giant star (2,352 words) [view diff] case mismatch in snippet view article find links to article

dwarf., § 4.1, 6.1. According to stellar evolution theory, no star of such low mass can have evolved to that stage within the age of the Universe. In stars

Ultra-cool dwarf (711 words) [view diff] case mismatch in snippet view article find links to article

Kirkpatrick, Todd J. Henry, and Michael J. Irwin. It originally included very low mass M-dwarf stars with spectral types of M7 but was later expanded to encompass

White dwarf (17,798 words) [view diff] case mismatch in snippet view article find links to article

oxygen–neon–magnesium (ONeMg or ONe) white dwarf may form. Stars of very low mass will be unable to fuse helium; hence, a helium white dwarf may form by

NGC 2244 (549 words) [view diff] no match in snippet view article find links to article

that otherwise would form low-mass stars or intermediate mass stars. The study also found a low disk fraction for low-mass objects of 39±9% for objects

2MASS (631 words) [view diff] no match in snippet view article find links to article

observed objects, including minor planets of the Solar System, brown dwarfs, low-mass stars, nebulae, star clusters and galaxies. In addition, 1 million objects

Protostar (1,238 words) [view diff] no match in snippet view article find links to article

cloud. It is the earliest phase in the process of stellar evolution. For a low-mass star (i.e. that of the Sun or lower), it lasts about 500,000 years. The

NGC 6535 (513 words) [view diff] case mismatch in snippet view article find links to article

75 billion years. For a object of its type, NGC 6535 has a relatively low mass of 2.2×104 times the mass of the Sun. The core radius is 2.3 ly (0.71 pc)

Stellar core (1,845 words) [view diff] no match in snippet view article find links to article

stars) the entire star is convective, including the core region. These very low-mass stars (VLMS) occupy the late range of the M-type main-sequence stars, or

Extreme helium star (728 words) [view diff] no match in snippet view article find links to article

An extreme helium star (abbreviated EHe) is a low-mass supergiant that is almost devoid of hydrogen, the most common chemical element of the Universe.

WR 136 (722 words) [view diff] no match in snippet view article find links to article

low-mass star of spectral classification K or M that would complete an orbit around the Wolf-Rayet star each 5.13 days, being the progenitor of a low-mass

Mercury (planet) (15,913 words) [view diff] no match in snippet view article

Mercury is the first planet from the Sun and the smallest in the Solar System. In English, it is named after the ancient Roman god Mercurius (Mercury)

NGC 4395 (850 words) [view diff] no match in snippet view article find links to article

active and the galaxy is classified as a Seyfert Type I known for its very low-mass supermassive black hole. NGC 4395 has a halo that is about 8′ in diameter

NGC 4845 (297 words) [view diff] no match in snippet view article find links to article

2013, the ESA observed the black hole absorbing matter from a nearby, low-mass object; possibly a brown dwarf star. The observed X-ray flare was caught

L1014 (309 words) [view diff] no match in snippet view article find links to article

star formation processes. This cloud harbors at its core a very young low-mass star named L1014 IRS; some astronomers have suggested that this object

Deuterium fusion (1,354 words) [view diff] no match in snippet view article find links to article

initial deuterium flash was proposed for very low-mass stars in 1964 by M. Gabriel. In this scenario a low-mass star or brown dwarf that is fully convective

NGC 4485 (340 words) [view diff] case mismatch in snippet view article find links to article

bridge of gas joining the two. Both galaxies are otherwise isolated and of low mass. The star formation rate in NGC 4485 is 0.22 M☉·yr−1. NGC 4485 and NGC

NGC 6712 (489 words) [view diff] no match in snippet view article find links to article

accompanied by a low-mass star or brown dwarf. The high amounts of radiation emitted from the pulsar contributes to the evaporation of the low-mass companion

SDSS J102915+172927 (606 words) [view diff] no match in snippet view article find links to article

fine structure cooling mechanism that is critical in the formation of low-mass stars, the origins of Caffau's Star are somewhat mysterious. It has been

XTE J1118+480 (696 words) [view diff] no match in snippet view article find links to article

XTE J1118+480 is a low-mass X-ray binary in the constellation Ursa Major. It is a soft X-ray transient that most likely contains a black hole and is probably

NGC 5806 (497 words) [view diff] case mismatch in snippet view article find links to article

2004dg has not been detected and is expected to have been a relatively low mass, low luminosity, red supergiant. The other supernovae are SN 2012P (type

G 196-3 (731 words) [view diff] no match in snippet view article find links to article

G 196-3 is a young low-mass M dwarf type star which is about 100 million years old. The star is located within the Ursa Major constellation about 71.1

UScoCTIO 108 (780 words) [view diff] no match in snippet view article find links to article

UScoCTIO 108A, with mass around 0.06 solar masses, is a brown dwarf or low-mass red dwarf. The secondary, UScoCTIO 108B, with a mass around the deuterium

NGC 3605 (268 words) [view diff] no match in snippet view article find links to article

discovered on March 14, 1784, by the astronomer William Herschel. A relatively low-mass galaxy, it is a member of the Leo II Group of galaxies, including NGC 3607

89 Herculis (666 words) [view diff] case mismatch in snippet view article find links to article

variable brightness and spectral line profiles. The companion has a very low mass and luminosity and orbits the primary in 288 days. The primary component

4U 0614+091 (121 words) [view diff] no match in snippet view article find links to article

4U 0614+091 is a low-mass X-ray binary star system which features a neutron star and a low-mass companion star. The binary system lies 10,000 light-years

OY Carinae (352 words) [view diff] no match in snippet view article find links to article

orbit each other every 1.51 hours, and possibly a yet unconfirmed third low-mass (substellar?) companion. Greenhill et al. (2009) would invoke the presence

AN Ursae Majoris (443 words) [view diff] case mismatch in snippet view article find links to article

known as polars. The pair consist of a low mass white dwarf with a strong magnetic field, interacting with a low–mass main sequence star that has filled its

NGC 157 (636 words) [view diff] case mismatch in snippet view article find links to article

rotation curve for this galaxy undergoes a sharp decline, suggesting a low mass or a small dark matter halo. It is considered a quiescent galaxy, showing

MOA-2007-BLG-192Lb (456 words) [view diff] no match in snippet view article find links to article

the constellation of Sagittarius. The planet was discovered orbiting the low-mass star MOA-2007-BLG-192L. It was found when it caused a gravitational microlensing

Subdwarf O star (564 words) [view diff] no match in snippet view article find links to article

A subdwarf O star (sdO) is a type of hot, but low-mass star. O-type subdwarfs are much dimmer than regular O-type main-sequence stars, but with a brightness

WASP-43b (1,838 words) [view diff] no match in snippet view article find links to article

Astrolábos, is a transiting planet in orbit around the young, active, and low-mass star WASP-43 in the constellation Sextans. The planet is a hot Jupiter

WISP (particle physics) (371 words) [view diff] no match in snippet view article

weakly interacting slender particle, or weakly interacting slim particle – low-mass particles which rarely interact with conventional particles. The term is

Bursting Pulsar (169 words) [view diff] no match in snippet view article find links to article

The Bursting Pulsar (GRO J1744-28) is a low-mass x-ray binary with a period of 11.8 days. It was discovered in December 1995 by the Burst and Transient

Elliptical galaxy (1,907 words) [view diff] no match in snippet view article find links to article

"early-type" galaxy population. Most elliptical galaxies are composed of older, low-mass stars, with a sparse interstellar medium, and they tend to be surrounded

NGC 1360 (326 words) [view diff] no match in snippet view article find links to article

1977, but was only confirmed in 2017. The central source consists of a low-mass O-type star and a white dwarf, with masses of 0.555 M☉ and 0.679 M☉ respectively

Flake salt (205 words) [view diff] case mismatch in snippet view article find links to article

Most form as thin, flattened out crystals with a large surface area and low mass that give them a crunchy texture and relatively fast dissolution rate.

Flake salt (205 words) [view diff] case mismatch in snippet view article find links to article

Most form as thin, flattened out crystals with a large surface area and low mass that give them a crunchy texture and relatively fast dissolution rate.

Cuspy halo problem (1,037 words) [view diff] no match in snippet view article find links to article

is a discrepancy between the inferred dark matter density profiles of low-mass galaxies and the density profiles predicted by cosmological N-body simulations

NGC 266 (469 words) [view diff] no match in snippet view article find links to article

spiral arms (ab). It is the dominant member of a small group with six low-mass galaxies. NGC 266 is an LINER-type active galaxy. It has a moderate star

V1027 Cygni (498 words) [view diff] no match in snippet view article find links to article

14,000 light years away. For a time, it was thought that it could be a low-mass post-AGB star, however recent parallax measurements published in Gaia DR3

LQ Andromedae (697 words) [view diff] no match in snippet view article find links to article

days. Not much is known about the secondary component, but it is likely a low-mass companion (M<0.5 M☉). A circumstellar disk is also present in the system

Proxima Centauri (10,215 words) [view diff] no match in snippet view article find links to article

Proxima Centauri is a small, low-mass star located 4.2465 light-years (1.3020 pc) away from the Sun in the southern constellation of Centaurus. Its Latin

2MASS 1237+6526 (402 words) [view diff] no match in snippet view article find links to article

light-years away from the Sun. The substellar object could likely host a very low-mass companion (yet undetected but inferred), possibly in the planetary regime

Saturn Nebula (665 words) [view diff] no match in snippet view article find links to article

his earliest discoveries in his sky survey. The nebula was originally a low-mass star that ejected its layers into space, forming the nebula. The central

Giant planet (2,657 words) [view diff] no match in snippet view article find links to article

of water, ammonia, and methane. The defining differences between a very low-mass brown dwarf and a massive gas giant (~13 MJ) are debated. One school of

Subgiant (3,704 words) [view diff] case mismatch in snippet view article find links to article

in the convective core. Low metallicity causes the central part of even low mass cores to be convectively unstable, and overshooting causes the core to

Swift J1745-26 (180 words) [view diff] no match in snippet view article find links to article

Swift J1745-26 in visible light. Swift J1745-26 must be a member of a low-mass X-ray binary (LMXB) system, which includes a normal, sun-like star. "SWIFT

DN Orionis (388 words) [view diff] case mismatch in snippet view article find links to article

in its spectrum. The pair have an unusually low mass ratio and the secondary appears to be of very low mass and overluminous. Mass is flowing from the

NGC 6642 (220 words) [view diff] no match in snippet view article find links to article

aging) have been spotted in this globular, and it is known to be lacking in low-mass stars. "SIMBAD query results". SIMBAD Astronomical Database. Retrieved

Habitability of neutron star systems (577 words) [view diff] no match in snippet view article find links to article

handful have sub-stellar companions. The most famous of these are the low-mass planets around the millisecond pulsar B1257+12. Habitability is conventionally

NGC 3621 (677 words) [view diff] case mismatch in snippet view article find links to article

active nucleus that matches a Seyfert 2 optical spectrum, suggesting that a low mass supermassive black hole is present at the core. Based upon the motion of

Aquila X-1 (369 words) [view diff] no match in snippet view article find links to article

Aquila X-1 (frequently abbreviated to Aql X-1) is a low-mass x-ray binary (LMXB) and the most luminous X-Ray source in the constellation Aquila. It was

HD 114613 (1,590 words) [view diff] no match in snippet view article find links to article

Keck-HIRES Eta-Earth low-mass planet search that also began in 2004. In Wittenmyer et al. 2012, HD 114613 is indicated to be a low-mass planet host. Though

25 Orionis (831 words) [view diff] no match in snippet view article find links to article

among a dense cluster of low-mass pre-main-sequence stars in the Orion OB1a. 25 Orionis is the dominant member of a rich low-mass star region, first identified

O-type star (3,350 words) [view diff] no match in snippet view article find links to article

supergiant stars, but also some central stars of planetary nebulae, old low-mass stars near the end of their lives, which typically have O-like spectra

LH 95 (341 words) [view diff] no match in snippet view article find links to article

typical stellar association in the LMC looks like. The large sample of low-mass pre–main sequence stars, stars that are currently under formation, in LH

List of stars in Scorpius (174 words) [view diff] no match in snippet view article find links to article

−33° 23′ 19.8″ low-mass X-ray binary GX 340+0 16h 45m 47.7s −45° 36′ 40″ low-mass X-ray binary H1743-322 17h 46m 15.61s −32° 14′ 00.6″ low-mass X-ray binary

2MASS J18082002−5104378 (823 words) [view diff] no match in snippet view article find links to article

entirely of materials released from the Big Bang. A tiny unseen companion, a low-mass UMP star, is particularly unusual. J1808−5104 is an ultra metal-poor (UMP)

Small planet radius gap (938 words) [view diff] no match in snippet view article find links to article

attributed to the absence of significant gas atmospheres on close-in, low-mass planets. This feature was noted as possibly confirming an emerging hypothesis

HD 4308 b (89 words) [view diff] no match in snippet view article find links to article

HD 4308 b is a low-mass exoplanet orbiting around HD 4308. It is believed to have almost no orbital eccentricity. HD 4203 b HD 4208 b Udry, S.; et al.

Gliese 876 d (1,210 words) [view diff] case mismatch in snippet view article find links to article

planets orbiting PSR B1257+12 at the time of its discovery. Due to its low mass, it can be categorized as a super-Earth. The mass of any exoplanet from

GRO J1719-24 (232 words) [view diff] case mismatch in snippet view article find links to article

a low-mass X-ray binary. Its name derives from an X-ray transient, detected in 1993. The system consists of a black hole candidate and a low mass companion

X-ray burster (1,608 words) [view diff] case mismatch in snippet view article find links to article

of the donor star; either a high mass (above 10 solar masses (M☉)) or low mass (less than 1 M☉) X-ray binary, abbreviated as HMXB and LMXB, respectively

NGC 6624 (310 words) [view diff] no match in snippet view article find links to article

was PSR J1823-3021A. This globular cluster also contains 4U 1820-30, a low-mass X-ray binary with an orbital period of only 11.5 minutes. NGC 6624 is visible

HD 65216 (657 words) [view diff] case mismatch in snippet view article find links to article

effective temperature of 5,718 K. In 2008 a co-moving binary system of low mass companions were discovered at an angular separation of 7″ from the primary

Main sequence (6,826 words) [view diff] no match in snippet view article find links to article

primarily by radiation, with a small core convection region. Medium-sized, low-mass stars like the Sun have a core region that is stable against convection

HD 85512 (759 words) [view diff] no match in snippet view article find links to article

Ceti. It exhibits a long-term variability and was thought to host one low-mass planet, although this is now doubtful. HD 85512 lies in Vela, 3′32″ west

F Hydrae (585 words) [view diff] case mismatch in snippet view article find links to article

rarely used since the star is now within the boundaries of Hydra. It is a low mass yellow supergiant around a thousand times brighter than the sun and five

Hen 2-437 (99 words) [view diff] case mismatch in snippet view article find links to article

first discovered by Rudolph Minkowski in 1946. Hen 2-437 formed when a low mass star similar to our sun swelled into its red giant phase ejecting its outer

HD 131399 (1,163 words) [view diff] no match in snippet view article find links to article

and further out are two lower-mass stars. A Jupiter-mass planet or a low-mass brown dwarf was once thought to be orbiting the central star, but this

NGC 7538 (282 words) [view diff] no match in snippet view article find links to article

several luminous near-IR and far-IR sources. Stars in NGC 7538 are mainly low-mass pre-main-sequence stars. Fallscheer; Reid; Di Francesco; Martin; Hill;

Super-Earth (7,202 words) [view diff] no match in snippet view article find links to article

8, 2010. Bennett, D. P.; et al. (2008). "Discovery of a Low-mass Planet Orbiting a Low-mass Star in Microlensing Event MOA-2007-BLG-192". Bulletin of

HD 35984 (358 words) [view diff] case mismatch in snippet view article find links to article

lithium may indicate that this is instead a weak-lined T Tauri star—a low mass pre-main sequence star that is relatively poor in circumstellar matter

K2-146b (266 words) [view diff] no match in snippet view article find links to article

exoplanet discovered in 2018 by the Kepler Space Telescope that orbits a low-mass M-type star in the constellation Cancer. Its host star, K2-146, is orbited

6 Boötis (517 words) [view diff] case mismatch in snippet view article find links to article

photosphere at an effective temperature of 4,050 K. Its companion is probably a low mass red dwarf of around class M8 V. Brown, A. G. A.; et al. (Gaia collaboration)

UY Volantis (761 words) [view diff] case mismatch in snippet view article find links to article

UY Volantis, also known as EXO 0748-676, is a low mass X-ray binary system located in the constellation Volans. With an apparent magnitude of 16.9, it

WZ Cephei (281 words) [view diff] no match in snippet view article find links to article

possible presence of a third low-mass stellar companion in a wide orbit. According to Zhu & Qian (2009) a third low-mass object of stellar nature could

HD 45350 b (441 words) [view diff] no match in snippet view article find links to article

Dynamical simulations covering a period of 107 years show that a second, low-mass, planet could only orbit stably if it were no more than 0.2 AU away from

HD 33636 (441 words) [view diff] no match in snippet view article find links to article

2002 with a minimum mass of planet size. This was ascertained to be a low-mass star in 2007, making it HD 33636 B. HD 33636 B was discovered in 2002 by

SAX J1808.4−3658 (329 words) [view diff] no match in snippet view article find links to article

making it a Rosetta stone for interpretation of the timing behavior of low-mass X-ray binaries. These accreting millisecond X-ray pulsars are thought to

PSR J1311–3430 (1,161 words) [view diff] case mismatch in snippet view article find links to article

of 93.8 minutes. The system is explained by a model where mass from the low mass companion was transferred on to the pulsar, increasing the mass of the

NGC 5053 (805 words) [view diff] case mismatch in snippet view article find links to article

are short period SX Phoenicis variable stars. NGC 5053 is a relatively low mass cluster with a low core concentration factor of 1.32. It sports a stream

NGC 5189 (509 words) [view diff] no match in snippet view article find links to article

finally found a white dwarf companion in a 4.04 day orbit around the rare low-mass Wolf-Rayet type central star of NGC 5189. NGC 5189 is estimated to be 546

Polar (star) (1,144 words) [view diff] no match in snippet view article

other CVs, polars contain two stars: an accreting white dwarf (WD), and a low-mass donor star (usually a red dwarf) which is transferring mass to the WD as

CP Puppis (588 words) [view diff] no match in snippet view article find links to article

a white dwarf that is accreting matter from a companion; most likely a low-mass main sequence star. This close binary system has an orbital period of 1

HD 53143 (764 words) [view diff] no match in snippet view article find links to article

conditions. Using the technique of gyrochronology, which measures the age of a low-mass star based on its rotation, HD 53143 is about 1,010 ± 130 million years

NGC 3741 (472 words) [view diff] no match in snippet view article find links to article

properties could be explained if NGC 3741 were a late-stage merger between a low-mass companion or if it accreted mass from the intergalactic medium. "NGC 3741"

NGC 7314 (554 words) [view diff] case mismatch in snippet view article find links to article

a type I Seyfert. The central supermassive black hole has a relatively low mass, estimated as (0.87±0.45)×106 M☉. The core is a source for X-ray emission

Polar (star) (1,144 words) [view diff] no match in snippet view article

other CVs, polars contain two stars: an accreting white dwarf (WD), and a low-mass donor star (usually a red dwarf) which is transferring mass to the WD as

List of exoplanets detected by microlensing (11,608 words) [view diff] no match in snippet view article find links to article

and a brown dwarf, with a low-mass planet orbiting the brown dwarf, but a model where the system consists of two low-mass stars with no planet was found

NGC 4660 (489 words) [view diff] no match in snippet view article find links to article

Alternatively, the detection of tidal dwarf galaxies (TDGs) which are “recycled” low-mass galaxies formed from interactions or mergers suggest that the filament

Star (16,412 words) [view diff] case mismatch in snippet view article find links to article

environment. Accordingly, astronomers often group stars by their mass: Very low mass stars, with masses below 0.5 M☉, are fully convective and distribute helium

Messier 21 (726 words) [view diff] no match in snippet view article find links to article

including many early B-type stars. An estimated 40–60 of the observed low-mass members are expected to be pre-main-sequence stars, with 26 candidates

CM Draconis (952 words) [view diff] case mismatch in snippet view article find links to article

system plays an important role in testing stellar structure models for very low mass stars. These comparisons find that models underpredict the stellar radii

CFBDSIR 2149−0403 (747 words) [view diff] no match in snippet view article find links to article

a free-floating planetary-mass object or possibly a high-metallicity, low-mass brown dwarf in the constellation Aquarius. Originally, it was thought to

NGC 3945 (462 words) [view diff] case mismatch in snippet view article find links to article

and luminosities, the central black hole of NGC 3945 has an unusually low mass, estimated to be around 9×106 M☉. However, it is also possible that NGC

T Persei (677 words) [view diff] case mismatch in snippet view article find links to article

secondary period. It is relatively inactive for the red supergiant star, with low mass loss rate 8×10−6 Solar_mass/year and no detectable dust shell. The Washington

Stellar collision (1,708 words) [view diff] no match in snippet view article find links to article

result of a stellar merger at the time. White dwarfs are the remnants of low-mass stars which, if they form a binary system with another star, can cause

NGC 5822 (529 words) [view diff] case mismatch in snippet view article find links to article

members lying within an angular radius of 22.1′. The cluster is considered low mass at ~1,700 times the mass of the Sun. It has a core radius of 1.1±0.1 pc

HD 8673 (691 words) [view diff] case mismatch in snippet view article find links to article

companion and it was concluded this was a false detection. However, a low mass stellar companion was detected in a wide orbit. This red dwarf star has

GX 339-4 (510 words) [view diff] no match in snippet view article find links to article

GX 339-4 is a moderately strong variable galactic low-mass X-ray binary (LMXB) source and black hole candidate that flares from time to time. From spectroscopic

Ross 458 (1,042 words) [view diff] no match in snippet view article find links to article

at a distance of 37.6 light-years from the Sun. Both of the stars are low-mass red dwarfs with at least one of them being a flare star. This binary system

Messier 12 (711 words) [view diff] no match in snippet view article find links to article

published in 2006 concluded that this cluster has an unusually low number of low-mass stars. The authors surmise that they were stripped from the cluster by

Microturbulence (467 words) [view diff] case mismatch in snippet view article find links to article

believed to be responsible for the observed turbulent velocity field, both in low mass stars and massive stars. When examined by a spectroscope, the velocity

HD 165634 (620 words) [view diff] no match in snippet view article find links to article

no excess of s-process elements such as barium. It may even have been a low-mass star that lost its envelope. Van Leeuwen, F. (2007). "Validation of the

W Ursae Majoris variable (494 words) [view diff] case mismatch in snippet view article find links to article

A W Ursae Majoris variable, also known as a low mass contact binary, is a type of eclipsing binary variable star. These stars are close binaries of spectral

Small satellite (4,201 words) [view diff] case mismatch in snippet view article find links to article

small satellite, miniaturized satellite, or smallsat is a satellite of low mass and size, usually under 1,200 kg (2,600 lb). While all such satellites

K2-288Bb (1,187 words) [view diff] no match in snippet view article find links to article

or mini-Neptune exoplanet orbiting in the habitable zone of K2-288B, a low-mass M-dwarf star in a binary star system in the constellation of Taurus about

GJ 3634 b (1,038 words) [view diff] no match in snippet view article find links to article

by a group of astronomers searching for exoplanets in the orbit of very-low-mass stars after the team reorganized their strategy, choosing to search for

Kepler-36b (213 words) [view diff] case mismatch in snippet view article find links to article

proximity of the planet to its host star combined with its relatively low mass caused the planet to lose all or most of its primordial hydrogen/helium

J. Davy Kirkpatrick (1,295 words) [view diff] no match in snippet view article find links to article

credited with first using the name "Tyche" to refer to a heretofore unseen, low-mass Solar companion in the Oort Cloud. He chose this term to be in direct contrast

Stellar nucleosynthesis (4,238 words) [view diff] no match in snippet view article find links to article

universe as the elements are contained within the star. Later in its life, a low-mass star will slowly eject its atmosphere via stellar wind, forming a planetary

List of nearest known black holes (1,219 words) [view diff] no match in snippet view article find links to article

Z.; Paradijs, J.; van den Heuvel, E.P.J. (July 2007), "A Catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)", Astronomy

Blue supergiant (2,494 words) [view diff] no match in snippet view article find links to article

the right of the main sequence. By analogy to the red giant branch for low-mass stars, this region is also called the blue giant branch. They are larger

MACHO-1997-BLG-41 (497 words) [view diff] no match in snippet view article find links to article

that the microlensing event could be interpreted as being caused by a low-mass binary system of two red dwarf stars located in the galactic disk if one

NGC 752 (452 words) [view diff] case mismatch in snippet view article find links to article

NGC 752. Since the age of the cluster is 1.34±0.06 Gyr, they are mainly low mass stars on the main sequence or red giants, with a main sequence turnoff

GS 2000+25 (334 words) [view diff] case mismatch in snippet view article find links to article

about 0.5 solar masses. Because the companion star has a low mass, the system is a low-mass X-ray binary. List of nearest black holes Chevalier, C.; Ilovaisky

Blue straggler (1,501 words) [view diff] case mismatch in snippet view article find links to article

identified in the Galactic halo, since all surviving main sequence stars are low mass. Several explanations have been put forth to explain the existence of blue

GR Muscae (260 words) [view diff] no match in snippet view article find links to article

a neutron star of between 1.2 and 1.8 times the mass of the Sun and a low-mass star likely to be around the mass of the Sun in close orbit. A magnitude

HR 4049 (1,066 words) [view diff] no match in snippet view article find links to article

Balmer series, to be a blue supergiant, although in reality it is an old low-mass star on the post-AGB phase of its life. Its atmosphere is extremely deficient

WASP-13b (1,049 words) [view diff] case mismatch in snippet view article find links to article

of Jupiter. This low relative mass might be caused by a core that is of low mass or that is not present at all. The planet orbits at approximately 5% of

NGC 6522 (802 words) [view diff] case mismatch in snippet view article find links to article

At present it trails the bar in its orbit around the core. This is a low mass globular cluster with an estimated 5.93×104 times the mass of the Sun.

3 Puppis (468 words) [view diff] case mismatch in snippet view article find links to article

which is unusual for an A-type star. It is thought to be caused by a low mass companion. The companion is calculated to be a B8III - B6V star with a

Gliese 569 (804 words) [view diff] case mismatch in snippet view article find links to article

either a low-mass star or a binary object. But with a mass about 8-9% that of the Sun means it may possibly be a binary of two extremely low mass ultra-cool

HD 114762 (813 words) [view diff] no match in snippet view article find links to article

estimated to be around 10 billion years old, although the properties of such low-mass stars are very similar across a wide range of ages. It is calculated have

K2-22b (400 words) [view diff] case mismatch in snippet view article find links to article

requires a low surface gravity from the host planet, implying it is a low mass, "Mars, Mercury, or even lunar sized bodies with surface gravities of 1/6

V603 Aquilae (911 words) [view diff] no match in snippet view article find links to article

Like all novae, it is a binary system, comprising a white dwarf and donor low-mass star in close orbit to the point of being only semidetached. The white

Red Square Nebula (421 words) [view diff] no match in snippet view article find links to article

could produce the nebula's shape: Towards the end of their lives, many low-mass stars, like the Sun, slough off their outer layers to produce striking

TW Hydrae (1,439 words) [view diff] no match in snippet view article find links to article

from the ALMA observatory. TW Hydrae is accompanied by about twenty other low-mass stars with similar ages and spatial motions, comprising the "TW Hydrae

China Dark Matter Experiment (489 words) [view diff] case mismatch in snippet view article find links to article

include scaling to CDEX-10 and CDEX-1T.[citation needed] CDEX-1 had first low mass results in 2013 and published limits on WIMP masses 6–20 GeV in 2014. Qian

Miniature Exoplanet Radial Velocity Array (473 words) [view diff] no match in snippet view article find links to article

planets orbiting the nearest low-mass stars "MINERVA-Red: An Intensive Survey for Planets Orbiting the Nearest Low-mass Stars to the Sun - Videos | Institute

Dwarf elliptical galaxy (808 words) [view diff] no match in snippet view article find links to article

ellipticals. An alternative suggestion is that dEs could be the remnants of low-mass spiral galaxies that obtained a rounder shape through the action of repeated

VW Cephei (363 words) [view diff] no match in snippet view article find links to article

suggest the presence of one more additional perturbing objects of likely low-mass stellar nature. Orbital period variations suggest the presence of one more

NGC 1333 (1,132 words) [view diff] case mismatch in snippet view article find links to article

or later has a disk. Scholz et al. argues that this indicates that very low mass PMOs form like planets (aka ejected planets) and not like stars (also called

HD 91312 (847 words) [view diff] no match in snippet view article find links to article

radial velocity as well as direct imaging, indicate the presence of a low-mass stellar companion. This companion is an early-to-mid red dwarf, and orbits

UW Coronae Borealis (355 words) [view diff] no match in snippet view article find links to article

UW Coronae Borealis, also known as MS 1603.6+2600, is a low-mass X-ray binary star system in the constellation Corona Borealis. Astronomer Simon Morris

QX Normae (220 words) [view diff] case mismatch in snippet view article find links to article

QX Normae is an active low mass X ray binary in the constellation Norma. It is composed of a neutron star and a star smaller and cooler than the Sun. The

V923 Aquilae (743 words) [view diff] case mismatch in snippet view article find links to article

modelled binary system shows a primary with a class of around B5–7e and a low mass secondary separated by around 250 times the radius of the Sun (250 R☉)

27 Hydrae (689 words) [view diff] no match in snippet view article find links to article

at an effective temperature of 4,965 K. The star is suspected to host a low-mass companion. The stellar companions to this star, designated components B

List of directly imaged exoplanets (3,806 words) [view diff] no match in snippet view article find links to article

Program. III. 2MASS J0249-0557 c: A Wide Planetary-mass Companion to a Low-mass Binary in the β Pic Moving Group". The Astronomical Journal. 156 (2): 57

HVS 7 (629 words) [view diff] no match in snippet view article find links to article

Hertzsprung–Russell diagram are expected to either be hot horizontal branch stars, low-mass helium-burning objects, or moderate mass hydrogen-burning stars slightly

FU Orionis star (615 words) [view diff] case mismatch in snippet view article find links to article

Orionis flare with abrupt mass transfer from an accretion disc onto a young, low mass T Tauri star. Mass accretion rates for these objects are estimated to be

NGC 1614 (862 words) [view diff] no match in snippet view article find links to article

75 Mpc. This galaxy is undergoing a minor merger event with a gas-rich, low-mass companion galaxy, located in a tidal tail to the southwest of the nucleus

Lacaille 8760 (1,006 words) [view diff] case mismatch in snippet view article find links to article

years ago when it came within 12 light-years (3.7 parsecs). Due to its low mass (60% of the Sun), it has an expected lifespan of about 75 billion (7.5

Gliese 674 (855 words) [view diff] no match in snippet view article find links to article

of the 200 million year old Castor stream of co-moving stars. This is a low-mass M-type main-sequence star with a stellar classification of M3V. The star

SN 2008ax (482 words) [view diff] case mismatch in snippet view article find links to article

is not favored by models which indicate the progenitor had a relatively low mass of 4–5 M☉ and extended hydrogen-rich atmosphere with a radius of 30–40 R☉

40 Cancri (531 words) [view diff] case mismatch in snippet view article find links to article

straggler. This is a second generation star formed through a collision of two low mass stars some 5–350 million years ago. The collision was either between two

Gamma Arietis (1,442 words) [view diff] case mismatch in snippet view article find links to article

Arietis system). γ1 Arietis may itself be a spectroscopic binary with a low mass companion. The combined apparent visual magnitude of the stars is 3.86

Inner moon (1,655 words) [view diff] case mismatch in snippet view article find links to article

parent planet, their short orbital periods (usually under a day), their low mass, small size, and irregular shapes. Thirty inner satellites are currently

45 Herculis (821 words) [view diff] no match in snippet view article find links to article

51 days on a moderately eccentric orbit. The secondary star is likely a low-mass star. Burke, E. W. Jr.; Barr, T. H. (June 1981). "Photometric UBV period

Gliese 180 (1,047 words) [view diff] no match in snippet view article find links to article

the HARPS M dwarf sample. The rotation-activity relationship for very low-mass stars through R'HK", Astronomy & Astrophysics, 600: 15, arXiv:1610.09007

J/psi meson (1,827 words) [view diff] no match in snippet view article find links to article

especially the low-mass flavorless mesons, not only because their very similar small masses can be easily confused, but also because the low-mass particles

1RXS J160929.1−210524 (1,319 words) [view diff] no match in snippet view article find links to article

simply a brown dwarf which formed in a manner similar to that of other low-mass and substellar companions. A 2013 study, using data from the Spitzer Space

ChaHα8 (284 words) [view diff] no match in snippet view article find links to article

hydrogen-alpha emission. It was discovered in 2000. It was found in 2007 to have a low-mass substellar companion in orbit around it via radial velocity observations

Gliese 623 (266 words) [view diff] no match in snippet view article find links to article

; Yamada, Ryan S.; Tuthill, Peter G. (2007). "Precision Masses of the Low-Mass Binary System GJ 623". The Astrophysical Journal. 661 (1): 496–501.

XTE J1550–564 (211 words) [view diff] no match in snippet view article find links to article

J1550-564, sometimes abbreviated to J1550 and also known as V381 Normae, is a low-mass X-ray binary in the constellation Norma. It is composed of a black hole

Theta Pegasi (925 words) [view diff] no match in snippet view article find links to article

a binary star due to an acceleration detected by Hipparcos. In 2021, a low-mass companion star was discovered, associated with θ Pegasi. It is a red dwarf

Nu Draconis (908 words) [view diff] case mismatch in snippet view article find links to article

eccentricity of 0.03. The primary is also an Am star, while the secondary has a low mass and luminosity and is only inferred from the orbital movement of the more

GRO J1655−40 (612 words) [view diff] no match in snippet view article find links to article

with several times the mass of the Sun. The optical companion of this low-mass X-ray binary is a subgiant F star. Along with GRS 1915+105, GRO J1655−40

X-ray astronomy (8,115 words) [view diff] no match in snippet view article find links to article

binaries although it falls on the borderline, ~2 M☉, between high- and low-mass X-ray binaries. In July 2020, astronomers reported the observation of a

List of smallest known stars (13,066 words) [view diff] no match in snippet view article find links to article

}} . Yue, Y. L.; Cui, X. H.; Xu, R. X. (2006-10-01). "Is PSR B0943+10 a low-mass quark star?". The Astrophysical Journal. 649 (2): L95–L98. arXiv:astro-ph/0603468

WASP-43 (878 words) [view diff] case mismatch in snippet view article find links to article

small orbit of WASP-43b is thought to be caused by WASP-43's unusually low mass. WASP-43 was first observed between January and May 2009 by the SuperWASP

HD 81817 (712 words) [view diff] no match in snippet view article find links to article

detection. If the latter mass estimate is correct, this object would be a low-mass star, probably a red dwarf. Further observations through 2022 have confirmed

Type II Cepheid (1,232 words) [view diff] case mismatch in snippet view article find links to article

and 50 days. They are population II stars: old, typically metal-poor, low mass objects. Like all Cepheid variables, Type IIs exhibit a relationship between

Pulsating white dwarf (1,988 words) [view diff] case mismatch in snippet view article find links to article

atmospheres, has also been proposed, and in May 2012, the first extremely low mass variable (ELMV) white dwarf was reported. These variables all exhibit small

Willman 1 (752 words) [view diff] no match in snippet view article find links to article

declared the least massive galaxy known, opening up a new category of ultra-low-mass galaxies, lower than the then-theoretical minimum of 10 million solar masses

47 Tucanae (1,930 words) [view diff] no match in snippet view article find links to article

variable stars containing white dwarfs accreting from companion stars, and low-mass X-ray binaries containing neutron stars that are not currently accreting

Z Chamaeleontis (519 words) [view diff] no match in snippet view article find links to article

eclipsing white dwarf and red dwarf and possibly a yet unconfirmed third low-mass substellar companion. Dai et al. (2009) invoke the presence of a third

Nebula (2,865 words) [view diff] no match in snippet view article find links to article

stellar winds or ultraviolet radiation from massive stars, or outflows from low-mass stars may disrupt the cloud, destroying the nebula after several million

WASP-19b (1,037 words) [view diff] no match in snippet view article find links to article

that of Jupiter, or 0.13 Solar radii); making it nearly the size of a low-mass star. It orbits the star WASP-19 in the Vela constellation. At the time

V1054 Ophiuchi (1,287 words) [view diff] case mismatch in snippet view article find links to article

detection of an infrared source near vB 8 suggested it had a low mass companion. The low mass of this candidate led to speculation that it may be a brown

List of X-ray pulsars (63 words) [view diff] no match in snippet view article find links to article

Low-mass binaries Spin period (sec) Orbital period (days) Companion (MK type) GRO J1744-28 0.467 11.8 unknown 4U 1626-67 7.66 0.0289 KZ TrA (low-mass

Messe de la Pentecôte (401 words) [view diff] exact match in snippet view article find links to article

himself wrote that the work "corresponds almost exactly with the length of a low Mass, and its sections are intended to match with those of the service. The

40 Leonis (643 words) [view diff] case mismatch in snippet view article find links to article

from this position, which may be coming from an undetected short-period, low mass companion. 40 Leonis has a common proper motion companion, NLTT 23781,

Sub-brown dwarf (1,328 words) [view diff] no match in snippet view article find links to article

Albert, Loïc (1 December 2020). "A Wide Planetary-mass Companion to a Young Low-mass Brown Dwarf in Ophiuchus". The Astrophysical Journal. 905 (2): L14. arXiv:2011

K2-28 (585 words) [view diff] no match in snippet view article find links to article

"Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. I. Classifying Low-mass Host Stars Observed during Campaigns 1–7". The Astrophysical

Walter Sagitta (401 words) [view diff] no match in snippet view article find links to article

inverted V-12 engine that first ran in 1937. This was one of several smaller, low-mass medium power pre-war V-12 engines produced. With a displacement of 18.4

List of stars in Triangulum Australe (232 words) [view diff] no match in snippet view article find links to article

8s −67° 27′ 43″ 18.50 Low-mass X-ray binary, Vmax = 18.23m, Vmin = 19m X1556-605 LU 16h 01m 02.3s −60° 44′ 18″ 18.60 Low-mass X-ray binary, Vmax = 18

70 Pegasi (577 words) [view diff] case mismatch in snippet view article find links to article

at an effective temperature of 5,108 K. The secondary is most likely a low mass main sequence star with no more than 0.4 times the mass of the Sun. van

NGC 2022 (652 words) [view diff] no match in snippet view article find links to article

from the Galactic Plane, which position suggests it was formed from a low-mass star. The elemental abundances are similar to those in the Sun, although

NGC 2022 (652 words) [view diff] no match in snippet view article find links to article

from the Galactic Plane, which position suggests it was formed from a low-mass star. The elemental abundances are similar to those in the Sun, although

R Sagittae (741 words) [view diff] case mismatch in snippet view article find links to article

that varies from magnitude 8.0 to 10.5 in 70.77 days. It is a post-AGB low mass yellow supergiant that varies between spectral types G0Ib and G8Ib as it

SWIFT J1756.9−2508 (261 words) [view diff] no match in snippet view article find links to article

of the accretion-powered millisecond pulsar SWIFT J1756.9-2508 with a low-mass companion". Astrophysical Journal Letters. 668 (2): L147–L150. arXiv:0709

Red giant (3,415 words) [view diff] case mismatch in snippet view article find links to article

contrary to their depiction in many illustrations. Rather, due to the very low mass density of the envelope, such stars lack a well-defined photosphere, and

Light dark matter (1,651 words) [view diff] case mismatch in snippet view article find links to article

where m is the WIMP mass and M the mass of the Z-boson. This means that low mass WIMPs, which would be abundantly produced in the early universe, freeze

HD 217786 (727 words) [view diff] no match in snippet view article find links to article

the Sun from its photosphere at an effective temperature of 5,882 K. A low-mass stellar companion at a projected separation of 155 AU was discovered in

Neutron cross section (2,865 words) [view diff] case mismatch in snippet view article find links to article

of all three. Isotopes which have a large scatter cross section and a low mass are good neutron moderators (see chart below). Nuclides which have a large

EZ Aquarii (1,141 words) [view diff] case mismatch in snippet view article find links to article

Xavier; et al. (October 1999). "Accurate masses of very low mass stars. II. The very low mass triple system GL 866". Astronomy and Astrophysics. 350:

IC 2602 (884 words) [view diff] no match in snippet view article find links to article

(1997). "Rotational Velocities and Chromospheric/Coronal Activity of Low-Mass Stars in the Young Open Clusters IC 2391 and IC 2602". Astrophysical Journal

RR Pictoris (806 words) [view diff] case mismatch in snippet view article find links to article

observed orbital period suggest that RR Pictoris system may include a low mass (0.25 M⊙) third star orbiting the close binary pair with a period of about

Starseed launcher (173 words) [view diff] case mismatch in snippet view article find links to article

nanocomputers. The required launch energy per probe would be low due to the low mass, and many nanoprobes would be launched in sequence and rendezvous in flight

Circumbinary planet (5,613 words) [view diff] no match in snippet view article find links to article

transiting exoplanet so far. A massive planet or brown dwarf around this low-mass X-ray binary (LMXB) system was found by the method of periodic delay in

EQ Tauri (1,107 words) [view diff] case mismatch in snippet view article find links to article

suggested it is caused by a third body in the system. They modeled it as a low mass red dwarf with an orbital period of 50.2 years. This is a shallow contact

PSR J1719−1438 (547 words) [view diff] no match in snippet view article find links to article

measurements using the Parkes Telescope and Lovell Telescope showed that it has a low-mass companion: PSR J1719-1438 b. The companion has a mass similar to that of

List of exoplanets discovered in 2017 (5,368 words) [view diff] no match in snippet view article find links to article

Ségransan, D.; Udry, S. (2017), "The Spitzersearch for the transits of HARPS low-mass planets", Astronomy & Astrophysics, 601: A117, arXiv:1701.01303, Bibcode:2017A&A

Theory of everything (6,472 words) [view diff] case mismatch in snippet view article find links to article

for understanding the universe in regions of both very small scale and low mass: subatomic particles, atoms, and molecules. Quantum mechanics successfully

Thermal lance (746 words) [view diff] case mismatch in snippet view article find links to article

oxygen because it has a high surface area-to-mass ratio and relatively low mass, which prevents the heat from being dissipated in the bulk of the material

Axion (7,625 words) [view diff] case mismatch in snippet view article find links to article

strong CP problem in quantum chromodynamics (QCD). If axions exist and have low mass within a specific range, they are of interest as a possible component of

Mini-Neptune (1,491 words) [view diff] no match in snippet view article find links to article

via hydrodynamic escape than larger planets and planets farther out. A low-mass gas planet can still have a radius resembling that of a gas giant if it

Kappa Delphini (422 words) [view diff] no match in snippet view article find links to article

orbital period of 45 years has been calculated. The secondary star is a low-mass star, at only 0.4 M☉. A third star is 12th magnitude ADS 14101 B, 10″ away

Methods of detecting exoplanets (15,274 words) [view diff] no match in snippet view article find links to article

detectable only in very small orbits around low-mass stars, e.g. Proxima b. It is easier to detect planets around low-mass stars, for two reasons: First, these

Rockoon (1,009 words) [view diff] no match in snippet view article find links to article

layers of the atmosphere. A 2016 study by Acta Astronautica concluded that low-mass and high altitude launches give the best results. The original concept

Spear-thrower (4,102 words) [view diff] no match in snippet view article find links to article

throwing arm together with the atlatl acts as a lever. The spear-thrower is a low-mass, fast-moving extension of the throwing arm, increasing the length of the

GQ Lupi (647 words) [view diff] no match in snippet view article find links to article

GQ Lupi b is listed as "confirmed planet" as in 2020. In 2020, another low-mass companion of GQ Lupi was discovered at a separation distance of about 16

Quantum tunnelling (6,474 words) [view diff] no match in snippet view article find links to article

the tunneling particle's mass, so tunneling is seen most prominently in low-mass particles such as electrons or protons tunneling through microscopically

Habitability of red dwarf systems (5,537 words) [view diff] no match in snippet view article find links to article

Pieter G.; Conroy, Charlie (1 December 2010). "A substantial population of low-mass stars in luminous elliptical galaxies". Nature. 468 (7326): 940–942. arXiv:1009

Millisecond pulsar (2,112 words) [view diff] no match in snippet view article find links to article

called recycled pulsars. Millisecond pulsars are thought to be related to low-mass X-ray binary systems. It is thought that the X-rays in these systems are

Fine Guidance Sensor (HST) (906 words) [view diff] no match in snippet view article

of astrometry science with the Hubble FGS system is observations of the Low-Mass Binary star system L722-22. Observations were taken of the system in 1990s

HD 117618 (718 words) [view diff] no match in snippet view article find links to article

the Anglo-Australian Planet Search program announced the discovery of a low-mass planet in orbit around HD 117618. This object was found through measurements

Nu Octantis (808 words) [view diff] case mismatch in snippet view article find links to article

star is likely either a red dwarf or a white dwarf, from its relatively low mass. This star is estimated to have around 60% the mass of the Sun. It shares

AI Velorum (1,223 words) [view diff] case mismatch in snippet view article find links to article

increase light emission. As an RR Lyrae variable, AI Velorum should be a low mass, evolved star. However, M. Breger in 1977 noted the period and surface

Subdwarf (2,103 words) [view diff] no match in snippet view article find links to article

Michael; Shara, Michael M. (November 2007). "Revised metallicity classes for low-mass stars: Dwarfs (dM), subdwarfs (sdM), extreme Subdwarfs (esdM), and ultrasubdwarfs

14 Trianguli (992 words) [view diff] no match in snippet view article find links to article

not been detected visually or in the spectrum and is expected to be a low-mass red dwarf or white dwarf. 14 Tri may be part of the Wolf 630 moving group

Epsilon Aurigae (3,599 words) [view diff] case mismatch in snippet view article find links to article

secondary with a mass over 13 M☉. The low mass model accepts the 5.9 M☉ secondary and so also requires a low-mass primary. The high-mass model accepts

Type II supernova (4,792 words) [view diff] no match in snippet view article find links to article

but not in elliptical galaxies; those are generally composed of older, low-mass stars, with few of the young, very massive stars necessary to cause a supernova

Helium planet (577 words) [view diff] no match in snippet view article find links to article

also get depleted. A helium-rich planetary object may also form from a low-mass white dwarf, which gets depleted of hydrogen via mass transfer in a close

Gliese 581d (3,109 words) [view diff] case mismatch in snippet view article find links to article

Earth masses), this super-Earth was the first exoplanet of relatively low mass regarded as orbiting within the habitable zone of its parent star. Assuming

TU Mensae (359 words) [view diff] no match in snippet view article find links to article

constellation Mensa. A close binary, it consists of a white dwarf and low-mass star orbiting each other in 2 hours 49 minutes. The stars are close enough

Proplyd (2,575 words) [view diff] no match in snippet view article find links to article

with these sources. Here the idea appeared that these objects might be low-mass stars surrounded by an evaporating protostellar accretion disk. Proplyds

Cryogenic Dark Matter Search (2,077 words) [view diff] no match in snippet view article find links to article

(called CDMSlite-mode) that was meant to be sensitive specifically to low-mass WIMPs. As the CDMS-experiment has multiple different detector technologies

Plutonium hexafluoride (2,920 words) [view diff] no match in snippet view article find links to article

uranium. This isotope of plutonium is needed to avoid premature ignition of low-mass nuclear weapon designs by neutrons produced by spontaneous fission of plutonium-240

2MASS J0523−1403 (829 words) [view diff] no match in snippet view article find links to article

2MASS J0523−1403 is a very-low-mass red dwarf about 40 light-years from Earth in the southern constellation of Lepus, with a very faint visual magnitude

LP 40-365 (360 words) [view diff] no match in snippet view article find links to article

LP 40-365 is a low-mass white dwarf star in the constellation Ursa Minor. It travels at high speed through the Milky Way and has a very unusual elemental

List of exoplanets discovered in 2019 (5,870 words) [view diff] no match in snippet view article find links to article

; Vines, J. I.; Suárez, Juan C.; Peña Rojas, P. A. (2019), "GJ 357: A low-mass planetary system uncovered by precision radial velocities and dynamical

Perseus molecular cloud (309 words) [view diff] no match in snippet view article find links to article

is almost invisible apart from two clusters, IC 348 and NGC 1333, where low-mass stars are formed. It is very bright at mid and far-infrared wavelengths

Gravitational microlensing (7,159 words) [view diff] no match in snippet view article find links to article

as the Hubble Space Telescope. With microlensing, the lens mass is too low (mass of a planet or a star) for the displacement of light to be observed easily

PICO (1,335 words) [view diff] no match in snippet view article find links to article

May 2012, using 10 detectors with total exposure 14 kg·d, to constrain low-mass WIMP interaction on 19F. The best spin-dependent limits were obtained for

X Crucis (546 words) [view diff] no match in snippet view article find links to article

a classical or type I Cepheid variable, to be distinguished from older low-mass stars called type II Cepheid variables. Classical Cepheids pulsate radially

SDSS J001820.5−093939.2 (1,364 words) [view diff] case mismatch in snippet view article find links to article

long enough to be discovered. The distinctive chemical patterns of these low mass stars can be used to estimate the mass of the first generation stars. In

Carbon planet (1,502 words) [view diff] no match in snippet view article find links to article

light-years), PSR J2222−0137 is a nearby intermediate-mass binary pulsar whose low-mass neutron star's companion is a white dwarf (PSR J2222−0137 B). The white

V404 Cygni (1,703 words) [view diff] no match in snippet view article find links to article

Cynthia S.; Robinson, Edward L. (2010). "Near-infrared Spectroscopy of Low-mass X-ray Binaries: Accretion Disk Contamination and Compact Object Mass Determination

GJ 3991 (445 words) [view diff] no match in snippet view article find links to article

secondary as a cold white dwarf star, the compact remnant that remains after a low-mass star such as the Sun is no longer able to fuse elements for energy. GJ

OGLE-2016-BLG-1190Lb (359 words) [view diff] case mismatch in snippet view article find links to article

with a mass about 13.4 times that of Jupiter (MJ), or is, possibly, a low mass brown dwarf, orbiting the G-dwarf star OGLE-2016-BLG-1190L, located about

1E 161348-5055 (394 words) [view diff] no match in snippet view article find links to article

increase in brightness. An alternate explanation is that the star has a low-mass X-ray binary. The companion star would orbit in an elongated orbit. When

HD 28185 (942 words) [view diff] no match in snippet view article find links to article

possibilities for habitable moons. In addition, numerical simulations suggest that low-mass planets located in the gas giant's Trojan points would be stable for long

Gliese 521 (711 words) [view diff] no match in snippet view article find links to article

A8. Jódar, Esther; et al. (February 2013). "New companions to nearby low-mass stars". Monthly Notices of the Royal Astronomical Society. 429 (1): 859–867

Planetary-mass object (1,994 words) [view diff] case mismatch in snippet view article find links to article

planetary-mass objects (iPMO; IPMO) are objects that are free-floating and have a low mass below deuterium burning and their nature as either an ejected free-floating

GRS 1915+105 (804 words) [view diff] no match in snippet view article find links to article

Q. Z; Van Paradijs, J; Van Den Heuvel, E. P. J (2007). "A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy

AB Doradus moving group (1,355 words) [view diff] no match in snippet view article find links to article

Lithium depletion and color-magnitude diagram positions amongst their low-mass members, suggesting that the two groups were of similar age (~100-125 Myr)

Ross 614 (669 words) [view diff] no match in snippet view article find links to article

which it is known. This binary star system consists of two closely spaced low-mass red dwarfs. The secondary star is a dim magnitude 14 lost in the glare

WISE 0146+4234 (317 words) [view diff] no match in snippet view article find links to article

Davy; et al. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal

VZ Piscium (1,332 words) [view diff] no match in snippet view article find links to article

projected separation of 1,825+180 −390 AU from the inner pair. It is a very low-mass star with 7.9–8.5% the mass of the Sun and a spectral type M9. This star

Dwarf star (578 words) [view diff] no match in snippet view article find links to article

main-sequence stars (dwarfs). Example: Achernar (B6Vep) Red dwarfs are low-mass main-sequence stars. Yellow dwarfs are main-sequence (dwarf) stars with

Candidate 1 (550 words) [view diff] no match in snippet view article find links to article

exoplanet candidate in a publication in Nature Communications titled “Imaging low-mass planets within the habitable zone of Alpha Centauri.” However, the observation

Soft X-ray transient (913 words) [view diff] no match in snippet view article find links to article

a black hole but sometimes a neutron star) and some type of "normal", low-mass star (i.e. a star with a mass of some fraction of the Sun's mass). These

Stellar black hole (4,019 words) [view diff] no match in snippet view article find links to article

solar masses. This is interpreted to suggest that there may be many such low-mass black holes that are not currently consuming any material and are hence

NGC 959 (607 words) [view diff] no match in snippet view article find links to article

Nicole C.; et al. (December 2019), "The Dark Matter Distributions in Low-mass Disk Galaxies. II. The Inner Density Profiles", The Astrophysical Journal

Exomoon (4,121 words) [view diff] case mismatch in snippet view article find links to article

satellites blurs the distinction between planets and moons, due to the low mass of brown dwarfs. This confusion is resolved by the International Astronomical

WISE J004945.61+215120.0 (379 words) [view diff] no match in snippet view article find links to article

Graeme (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal

Beta Crateris (1,099 words) [view diff] case mismatch in snippet view article find links to article

has been cooling down for around four million years. It has an unusually low mass, 43% that of the Sun, suggesting that the white dwarf progenitor may have

DL Tauri (569 words) [view diff] case mismatch in snippet view article find links to article

DL Tauri. The object is either a sub-brown dwarf or a low mass brown dwarf or even a low-mass ultra-cool red dwarf star if strongly veiled by accretion

Gliese 687 (790 words) [view diff] no match in snippet view article find links to article

"First Results from the CHARA Array. IV. The Interferometric Radii of Low-Mass Stars". The Astrophysical Journal. 644 (1): 475–483. arXiv:astro-ph/0602105

Epsilon Coronae Australis (632 words) [view diff] case mismatch in snippet view article find links to article

4.74 to 5 over 14 hours, it is the brightest W Ursae Majoris variable (low mass contact binary) in the night sky. Nicolas Louis de Lacaille gave Epsilon

Groombridge 1618 (1,558 words) [view diff] case mismatch in snippet view article find links to article

Forveille, Thierry; Queloz, Didier (2003). "First radius measurements of very low mass stars with the VLTI". Astronomy and Astrophysics. 397 (3): L5–L8. arXiv:astro-ph/0211647

2MASS J05325346+8246465 (600 words) [view diff] no match in snippet view article find links to article

Gálvez-Ortiz, M. C.; Burgasser, A. J.; Zhang (张曾华), Z. H. (2019), "Primeval very low-mass stars and brown dwarfs – VI. Population properties of metal-poor degenerate

GU Piscium (373 words) [view diff] no match in snippet view article find links to article

(2014). "BANYAN. III. Radial Velocity, Rotation, and X-Ray Emission of Low-mass Star Candidates in Nearby Young Kinematic Groups". The Astrophysical Journal

Wolf 359 (3,947 words) [view diff] case mismatch in snippet view article find links to article

conjunction with a much lower rate of hydrogen consumption due to its low mass and core temperature, Wolf 359 is expected to remain a main sequence star

NGC 1553 (1,037 words) [view diff] no match in snippet view article find links to article

gas making up 70% of the emissions, dotted with many point-like sources (low-mass X-ray binaries) making up the rest. Similarly to NGC 4697 and Messier 60

HD 1461 b (220 words) [view diff] no match in snippet view article find links to article

S2CID 12840404. Tim Stephens (2009-12-13). "New planet discoveries suggest low-mass planets are common around nearby stars". UCSC News. UC Santa Cruz. Retrieved

HAT-P-13 (722 words) [view diff] case mismatch in snippet view article find links to article

Because of its mass, this companion could either be a massive planet or a low mass brown dwarf. Either way, HAT-P-13 c orbits its sun every 446 days in a

Boron suboxide (1,030 words) [view diff] case mismatch in snippet view article find links to article

great hardness (close to that of rhenium diboride and boron nitride), low mass density, high thermal conductivity, high chemical inertness, and excellent

Lambda Orionis Cluster (760 words) [view diff] no match in snippet view article find links to article

million years. The star cluster is young and contains a large number of low-mass stars, some T Tauri stars and brown dwarfs. One notable member is LOri167

WD 1337+705 (575 words) [view diff] case mismatch in snippet view article find links to article

discovered magnesium in its spectrum, which suggests that it has some low mass companion or accretion of material happening as the star's temperature

ANAIS-112 (3,696 words) [view diff] no match in snippet view article find links to article

; Araujo, G. R.; Asner, D. M.; Ave, M.; Back, H. O. (23 August 2018). "Low-Mass Dark Matter Search with the DarkSide-50 Experiment". Physical Review Letters

List of nearest exoplanets (7,640 words) [view diff] no match in snippet view article find links to article

Del Sordo, Fabio; Anglada-Escudé, Guillem; et al. (15 January 2020). "A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU". Science

Stellar population (3,549 words) [view diff] no match in snippet view article find links to article

their metallic composition. This also explains why there have been no low-mass stars with zero metallicity observed, despite models constructed for smaller

Tyche (hypothetical planet) (1,605 words) [view diff] no match in snippet view article

S2CID 118513110. Bruce Dorminey (March 31, 2013). "Sun May Still Have Low-Mass Solar Companion, Say Astrophysicists Searching NASA WISE Mission Data"

R Coronae Borealis (2,228 words) [view diff] no match in snippet view article find links to article

R Coronae Borealis is a low-mass yellow supergiant star in the constellation of Corona Borealis. It is the prototype of the R Coronae Borealis variable

AD Leonis (1,819 words) [view diff] no match in snippet view article find links to article

Evgenya; Liu, Michael C.; Reid, I. Neill (July 2009). "Identifying the young low-mass stars within 25 pc. I. Spectroscopic observations". The Astrophysical Journal

List of planet types (547 words) [view diff] no match in snippet view article find links to article

Earth's deserts. Mars is arguably an example of a desert planet. Gas dwarf A low-mass planet composed primarily of hydrogen and helium. Gas giant A massive planet

HD 82514 (853 words) [view diff] case mismatch in snippet view article find links to article

CD −35°5751BC, which makes it a double star itself. It consists of two low mass stars separated by 2.3 " from each other. However, the system is not related

List of red dwarfs (839 words) [view diff] no match in snippet view article find links to article

Maxted, Pierre F. L. (August 2017). "The EBLM project III. A Saturn-size low-mass star at the hydrogen-burning limit". Astronomy & Astrophysics. 604: L6

List of planet types (547 words) [view diff] no match in snippet view article find links to article

Earth's deserts. Mars is arguably an example of a desert planet. Gas dwarf A low-mass planet composed primarily of hydrogen and helium. Gas giant A massive planet

RU Lupi (896 words) [view diff] no match in snippet view article find links to article

larger. This is a T Tauri star, which is a stage that a newly formed, low-mass star passes through before settling down onto the main sequence, where

Pre-stellar core (199 words) [view diff] no match in snippet view article find links to article

the nurseries of new stars, and are an early phase in the formation of low-mass stars, before gravitational collapse produces a central protostar. The

Nebular hypothesis (9,132 words) [view diff] no match in snippet view article find links to article

of the Solar System. Primitive-type meteorites are chunks of shattered low-mass planetesimals, where no thermal differentiation took place, while processed-type

38 Aurigae (570 words) [view diff] no match in snippet view article find links to article

Saurav; et al. (2010), "Sloan Low-mass Wide Pairs of Kinematically Equivalent Stars (SLoWPoKES): A Catalog of Very Wide, Low-mass Pairs", The Astronomical

English Missal (629 words) [view diff] exact match in snippet view article find links to article

English Missal is used for Low Mass on Fridays. St Mary Magdalen, Coventry Coventry The English Missal is used for Low Mass on Tuesdays at 6pm. St Magnus

Beta Caeli (584 words) [view diff] no match in snippet view article find links to article

rotational velocity of around 97.5 km/s. The companion is likely to be a low-mass (0.2 M☉) star orbiting about 5 AU from the primary. This object may be

WISE J0005+3737 (380 words) [view diff] no match in snippet view article find links to article

Graeme (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal

Meissa (1,766 words) [view diff] case mismatch in snippet view article find links to article

star with a classification of F8 V. This star in turn may have a very low mass companion that is probably a brown dwarf. Meissa is surrounded by a ring

WISEPA J173835.53+273258.9 (1,128 words) [view diff] case mismatch in snippet view article find links to article

1405+5534. Disequilibrium chemistry models suggest that this Y-dwarf has a low mass of about 3-9 MJup, making it a possible isolated planetary-mass object

THESEUS (562 words) [view diff] no match in snippet view article find links to article

on the cosmic star formation rate, the number density and properties of low-mass galaxies, the neutral hydrogen fraction, and the escape fraction of ultraviolet

Gamma Ceti (1,664 words) [view diff] no match in snippet view article find links to article

J. (7 May 2010). "Sloan Low-mass Wide Pairs of Kinematically Equivalent Stars (SLoWPoKES): A Catalog of Very Wide, Low-mass Pairs". The Astronomical

Gum Nebula (545 words) [view diff] no match in snippet view article find links to article

image. CG 4 Barnard's Loop Graham, J.A., 1986. Objects associated with low-mass star formation in the Gum nebula. The Astrophysical Journal, 302, pp.352-362

Air well (condenser) (5,330 words) [view diff] no match in snippet view article

High-mass air wells: used in the early 20th century, but the approach failed. Low-mass, radiative collectors: Developed in the late 20th century onwards, proved

IC 2391 (1,238 words) [view diff] no match in snippet view article find links to article

(1997). "Rotational Velocities and Chromospheric/Coronal Activity of Low-Mass Stars in the Young Open Clusters IC 2391 and IC 2602". Astrophysical Journal

Ballute (1,398 words) [view diff] no match in snippet view article find links to article

Various proposals involving ballutes, such as for deorbiting/recovering low-mass satellites and interplanetary research programmes, have been issued in

HD 42936 (737 words) [view diff] case mismatch in snippet view article find links to article

metal enriched despite an age of 10.9 billion years. HD 42936 has a very low mass companion star in a close orbit, approaching to 0.498 AU at periastron

Discoveries of exoplanets (8,227 words) [view diff] no match in snippet view article find links to article

planets around HD 1461 were discovered. These discoveries indicated that low-mass planets that orbit around nearby stars are very common. 61 Virginis is

HD 23514 (439 words) [view diff] no match in snippet view article find links to article

Andrew W.; Flagg, Laura (2015-06-09). "Planets Around Low-Mass Stars (PALMS). V. Age-Dating Low-Mass Companions to Members and Interlopers of Young Moving

Supergiant (5,371 words) [view diff] case mismatch in snippet view article find links to article

can be comparable to more massive red supergiants, but because of their low mass, being in a different stage of development (helium shell burning), and

Gyrochronology (881 words) [view diff] no match in snippet view article find links to article

Gyrochronology is a method for estimating the age of a low-mass (cool) main sequence star (spectral class F8 V or later) from its rotation period. The

Viktor Safronov (253 words) [view diff] no match in snippet view article find links to article

September 1999 in Moscow, Russia) was a Soviet astronomer who put forward the low-mass-nebula model of planet formation, a consistent picture of how the planets

PSR B0943+10 (695 words) [view diff] no match in snippet view article find links to article

University published a paper suggesting that the pulsar may actually be a low-mass quark star with mass around 0.02 M☉. In May 2014, two gas giants were found

WISE J080822.18-644357.3 (1,056 words) [view diff] no match in snippet view article find links to article

while being in an older moving group. Together with J0808, these older low-mass accretors in nearby moving groups are being called Peter Pan disks. Spectral

List of stars in Norma (98 words) [view diff] no match in snippet view article find links to article

78618 d 4U 1624-490 16h 28m 02.83s −49° 11′ 54.6″ Low-mass X-ray binary 4U 1630-47 16h 34m 01.61s −47° 23′ 34.8″ Low-mass X-ray binary Table legend:

Red-giant branch (3,933 words) [view diff] no match in snippet view article find links to article

evolving towards red giants, in contrast to the short densely populated low-mass subgiant branch seen in older clusters such as ω Centauri. Stars at the

HD 117618 b (225 words) [view diff] no match in snippet view article find links to article

simultaneously named "Dofida" in the contest. Tinney, C. G.; et al. (2005). "Three Low-Mass Planets from the Anglo-Australian Planet Search". The Astrophysical Journal

NGC 300 (1,941 words) [view diff] no match in snippet view article find links to article

accurate upper bound on the progenitor star's brightness. This suggested a low-mass main sequence star as progenitor with the transient resulting from a stellar

WISE 1534–1043 (1,337 words) [view diff] no match in snippet view article find links to article

for late T and Y-dwarfs. Alternative explanations include an extremely low-mass and young brown dwarf. This scenario cannot explain the high velocity,

List of stars in Circinus (133 words) [view diff] no match in snippet view article find links to article

13h 58m 09.92s −64° 44′ 04.9″ 16.9 low-mass X-ray binary Circinus X-1 BR 15h 20m 40.85s −57° 10′ 00.1″ 21.4 low-mass X-ray binary PSR B1451-68 14h 56m

St Matthew's Church, Willesden (443 words) [view diff] exact match in snippet view article find links to article

11am; Monday - Low Mass at 10am; Tuesday - Low Mass at 10am; Wednesday - Low Mass at 7.30pm; Thursday - Low Mass at 12noon; Friday - Low Mass at 10am. Chancel

Iron planet (628 words) [view diff] no match in snippet view article find links to article

Density, Ultra-short Period Sub-Earth GJ 367 b: Discovery of Two Additional Low-mass Planets at 11.5 and 34 Days". The Astrophysical Journal Letters. 955 (1):

WZ Andromedae (520 words) [view diff] case mismatch in snippet view article find links to article

An alternative explanation could be the presence in the system of two low mass companions with orbital periods of 50 and 70 years, respectively. Their

AFGL 2591 (254 words) [view diff] no match in snippet view article find links to article

Shepherd, D. S.; Robitaille, T. P.; Wood, K. (2013). "The standard model of low-mass star formation applied to massive stars: a multi-wavelength picture of

Exoplanet (15,942 words) [view diff] no match in snippet view article find links to article

April 2014 are massive and have wide orbits so probably represent the low-mass end of a brown dwarf formation. One study suggests that objects above 10 MJup

Sigma Coronae Borealis (1,476 words) [view diff] no match in snippet view article find links to article

star system containing three sunlike main-sequence stars and two other low-mass stars. The combined visual magnitude is 5.3 and the system lies 74 light

Ross 154 (1,384 words) [view diff] no match in snippet view article find links to article

abundance of elements heavier than helium is about half that in the Sun. No low-mass companions have been discovered in orbit around Ross 154. Nor does it display

IC 2149 (302 words) [view diff] no match in snippet view article find links to article

mass of 0.03 solar masses and being thought to have been produced by a low-mass star. Some authors have proposed the planetary nebula that the Sun will

PSR J0437−4715 (619 words) [view diff] no match in snippet view article find links to article

indicate that the binary companion of PSR J0437-4715 is most likely a low-mass helium white dwarf. The pulsar is about 1.4 solar mass (M☉) and the companion

Kepler object of interest (2,394 words) [view diff] case mismatch in snippet view article find links to article

exhibit such behavior. KOI-126 is a triple star system comprising two low mass (0.24 and 0.21 solar masses (M☉)) stars orbiting each other with a period

Trapezium Cluster (847 words) [view diff] no match in snippet view article find links to article

likely precursor to planetary formation. In addition, brown dwarfs and low-mass runaway stars have been identified. A 2012 paper suggests an intermediate-mass

EDELWEISS (952 words) [view diff] case mismatch in snippet view article find links to article

a total effective exposure of 384 kg·d) limiting high mass: Fig 5 and low mass WIMPs, and axions. A cross-section of 4.4×10−8 pb is excluded at 90% C

Tolman–Oppenheimer–Volkoff limit (3,144 words) [view diff] no match in snippet view article find links to article

A.; Kochanek, C. S.; Stanek, K. Z.; et al. (2019). "A noninteracting low-mass black hole–giant star binary system". Science. 366 (6465): 637–640. arXiv:1806

Beehive Cluster (1,932 words) [view diff] no match in snippet view article find links to article

DJ; Dobbie PD; Jameson F; Steele IA; et al. (2003). "Brown dwarfs and low-mass stars in the Pleiades and Praesepe: Membership and binarity". Monthly Notices

AW Ursae Majoris (1,939 words) [view diff] case mismatch in snippet view article find links to article

Mochnacki and N. A. Doughty modelled the system and determined a very low mass ratio of 0.079±0.08 for the pair, indicating that the secondary has 8%

Tolman–Oppenheimer–Volkoff limit (3,144 words) [view diff] no match in snippet view article find links to article

A.; Kochanek, C. S.; Stanek, K. Z.; et al. (2019). "A noninteracting low-mass black hole–giant star binary system". Science. 366 (6465): 637–640. arXiv:1806

List of Anglo-Catholic churches (2,067 words) [view diff] exact match in snippet view article find links to article

with "full Catholic privileges" – Solemn Mass and the Angelus on Sundays; Low Mass during the week and on Holy Days; regular time for confessions; holy water

Neutron star (13,793 words) [view diff] no match in snippet view article find links to article

"accretion-powered pulsars": a class of X-ray binaries. Low-mass X-ray binary pulsars: a class of low-mass X-ray binaries (LMXB), a pulsar with a main sequence

List of stars in Corona Borealis (95 words) [view diff] no match in snippet view article find links to article

18 57 G2V has a companion, has two planets (b & c), now thought to be a low-mass star. ν2 CrB ν2 21 147767 80214 16h 22m 29.22s +33° 42′ 12.1″ 5.40 −0.72

S Ori 70 (964 words) [view diff] no match in snippet view article find links to article

Osorio's T-type brown dwarf discovery and its spectroscopically verified low-mass. A comparison of the J band spectrum between S Ori 70 and other field objects

S-process (2,215 words) [view diff] no match in snippet view article find links to article

lowest metallicity stars. The production sites of the main component are low-mass asymptotic giant branch stars. The main component relies on the 13C neutron

List of nearest terrestrial exoplanet candidates (1,816 words) [view diff] no match in snippet view article find links to article

"The HARPS search for Earth-like planets in the habitable zone: I – Very low-mass planets around HD20794, HD85512 and HD192310", Astronomy & Astrophysics

HD 102117 b (247 words) [view diff] no match in snippet view article find links to article

using the radial velocity method. Tinney, C. G.; et al. (2005). "Three Low-Mass Planets from the Anglo-Australian Planet Search". The Astrophysical Journal

K2-33 (1,317 words) [view diff] case mismatch in snippet view article find links to article

observational limits only allows for the existence of brown dwarfs or very low mass stars at separations of 1-3 AU. The only known planet transits the star;

Korea Invisible Mass Search (999 words) [view diff] no match in snippet view article find links to article

signal reports for masses above 20 GeV. Using 24,324.3 kg•days exposure, low-mass WIMP signals below 20 GeV were disfavored in 2014. The KIMS and DM-Ice

List of exoplanet extremes (4,864 words) [view diff] no match in snippet view article find links to article

Kelle L. (18 February 2014). "Accretion Onto Planetary Mass Companions of Low-Mass Young Stars". The Astrophysical Journal. 783 (1): L17. arXiv:1401.6545

Backyard Worlds (4,677 words) [view diff] no match in snippet view article find links to article

old). The backyard worlds project found additional co-moving systems. 34 low-mass co-moving companions were discovered in 2022 with the NOIRLab Source Catalog

Chamaeleon (657 words) [view diff] no match in snippet view article find links to article

number of molecular clouds (the Chamaeleon dark clouds) that are forming low-mass T Tauri stars. The cloud complex lies some 400 to 600 light years from

NGC 4647 (536 words) [view diff] no match in snippet view article find links to article

Jimmy A. (5 September 2005). "XMM-Newton Observation of Diffuse Gas and Low-Mass X-Ray Binaries in the Elliptical Galaxy NGC 4649 (M60)". The Astrophysical

NGC 4458 (646 words) [view diff] no match in snippet view article find links to article

Jay (2017-11-13). "Detection of Enhanced Central Mass-to-light Ratios in Low-mass Early-type Galaxies: Evidence for Black Holes?". The Astrophysical Journal

Cathode ray (2,648 words) [view diff] case mismatch in snippet view article find links to article

empty tube. The voltage applied between the electrodes accelerates these low mass particles to high velocities. Cathode rays are invisible, but their presence

HD 104237 (1,427 words) [view diff] case mismatch in snippet view article find links to article

observations combined with the Chandra X-ray Observatory indicated that five low mass, pre-main sequence objects lie within 5″, equivalent to a projected distance

Lacaille 9352 (1,118 words) [view diff] no match in snippet view article find links to article

Bruno; Petrov, Romain (October 2009). "Mass-radius relation of low and very low-mass stars revisited with the VLTI". Astronomy and Astrophysics. 505 (1): 205–215

Soyuz MS-05 (440 words) [view diff] case mismatch in snippet view article find links to article

returning to the ground, together with the crew, payloads of relatively low mass and volume disposal of wastes from the station in the living compartment

Planetary migration (5,112 words) [view diff] case mismatch in snippet view article find links to article

dissipates. Interactions with leftover planetesimals can break resonances of low mass planets leaving them in orbits slightly outside the resonance. Tidal interactions

HD 43848 (336 words) [view diff] no match in snippet view article find links to article

2048G, doi:10.1086/378365, S2CID 119417105 Minniti, Dante; et al. (2009), "Low-Mass Companions for Five Solar-Type Stars From the Magellan Planet Search Program"

V1191 Cygni (942 words) [view diff] case mismatch in snippet view article find links to article

B.; Kalomeni, B.; Keskin, V.; Köse, O.; Yakut, K. (2012). "Marginally low mass ratio close binary system V1191 Cyg". New Astronomy. 17 (1): 46–49. arXiv:1107

OGLE-TR-113b (326 words) [view diff] no match in snippet view article find links to article

star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet, radial velocity measurements

Jupiter mass (1,261 words) [view diff] case mismatch in snippet view article find links to article

; Lunine, Jonathan I. (1993). "An expanded set of brown dwarf and very low mass star models". Astrophysical Journal. 406 (1): 158–71. Bibcode:1993ApJ.

OGLE-TR-111b (390 words) [view diff] no match in snippet view article find links to article

object had not been measured, it was not clear that it was a true planet, low-mass red dwarf or something else. In 2004 radial velocity measurements showed

17 Cygni (863 words) [view diff] no match in snippet view article find links to article

et al. (June 2010), "Sloan Low-mass Wide Pairs of Kinematically Equivalent Stars (SLoWPoKES): A Catalog of Very Wide, Low-mass Pairs", The Astronomical

Flare star (1,815 words) [view diff] case mismatch in snippet view article find links to article

powerful than the largest observed solar flare. TVLM 513-46546 is a very low mass M9 flare star, at the boundary between red dwarfs and brown dwarfs. Data

Gliese 22 (782 words) [view diff] no match in snippet view article find links to article

D. W.; Henry, Todd J.; McLeod, Brian; Christou, Julian C. (1991). "The Low-Mass Companion of Gliese 22A: First Results of the Steward Infrared Speckle

List of particles (2,981 words) [view diff] case mismatch in snippet view article find links to article

A WISP (weakly interacting slender particle) is any one of a number of low mass particles that might explain dark matter (such as the axion) A GIMP (gravitationally

61 Virginis (1,931 words) [view diff] no match in snippet view article find links to article

"Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems". MNRAS. 424 (2): 1206–1223. arXiv:1206.2370. Bibcode:2012MNRAS

Aeroponics (6,989 words) [view diff] no match in snippet view article find links to article

imbalance within the air culture system. To address this issue, special low-mass polymer materials have been developed and are utilized to prevent mineralization

Phoenix (constellation) (3,667 words) [view diff] no match in snippet view article

; et al. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal

HD 92788 (635 words) [view diff] no match in snippet view article find links to article

method. Designated component 'b', it is a Super-Jupiter or possibly a low-mass brown dwarf with an orbital period of 0.89 years. The star rotates at an

Orion Nebula (4,810 words) [view diff] no match in snippet view article find links to article

with these sources. Here the idea appeared that these objects might be low-mass stars surrounded by an evaporating protostellar accretion disk. In 1993

AZ Cancri (1,355 words) [view diff] no match in snippet view article find links to article

approximately 14.0 parsecs (46 ly) from the Sun, and is considered a very low-mass star with a radial velocity of 64.2±0.6 km/s. AZ Cancri belongs kinematically

Teegarden's Star (1,816 words) [view diff] no match in snippet view article find links to article

March 2022). "Rotational Modulation of Spectroscopic Zeeman Signatures in Low-mass Stars". The Astrophysical Journal. 927 (1): 11. arXiv:2201.11288. Bibcode:2022ApJ

Planet-hosting star (3,510 words) [view diff] no match in snippet view article find links to article

stars are successively higher towards cooler, less massive stars. At the low-mass end of star-formation are sub-stellar objects that do not fuse hydrogen:

Gliese 105 (1,203 words) [view diff] exact match in snippet view article find links to article

Retrieved 4 June 2017. Golimowski, David A.; et al. (2000). "The Very Low Mass Component of the Gliese 105 System". The Astronomical Journal. 120 (4):

Exoplanet interiors (2,407 words) [view diff] no match in snippet view article find links to article

its formation. A fast cooling rate is expected for a smaller planet, a low-mass planet, or a planet that is further away from its star. Such planets would

Coatlicue (star) (336 words) [view diff] no match in snippet view article

from stable isotopes and 10Be for solar system formation triggered by a low-mass supernova". Nature Communications. 7: 13639. arXiv:1611.07162. Bibcode:2016NatCo

TW Horologii (835 words) [view diff] no match in snippet view article find links to article

binary star system. An analysis of the motion of TW Horologii suggests a low-mass companion, although the UV excess suggests it is hot. In 2013 the luminosity

OGLE-TR-132b (306 words) [view diff] no match in snippet view article find links to article

star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements

Chi Capricorni (760 words) [view diff] no match in snippet view article find links to article

et al. (June 2010), "Sloan Low-mass Wide Pairs of Kinematically Equivalent Stars (SLoWPoKES): A Catalog of Very Wide, Low-mass Pairs", The Astronomical

Black dwarf (1,142 words) [view diff] no match in snippet view article find links to article

Retrieved 3 May 2007. Richmond, Michael. "Late stages of evolution for low-mass stars". Rochester Institute of Technology. Retrieved 4 August 2006. Alcock

Quark star (3,070 words) [view diff] no match in snippet view article find links to article

from Peking University, suggested that PSR B0943+10 may in fact be a low-mass quark star. It was reported in 2008 that observations of supernovae SN

Planetary habitability (13,145 words) [view diff] case mismatch in snippet view article find links to article

necessary to generate Earth's magnetic field. "Low mass" is partly a relative label: the Earth is low mass when compared to the Solar System's gas giants

RV Tauri variable (1,539 words) [view diff] no match in snippet view article find links to article

luminosity classes are due to very low surface gravities on pulsating low-mass and rarefied stars. RV Tauri variables are very luminous stars and are

List of brown dwarfs (3,653 words) [view diff] no match in snippet view article find links to article

dwarfs. These are objects that have masses between heavy gas giants and low-mass stars. The first isolated brown dwarf discovered was Teide 1 in 1995. The

Light curve (1,513 words) [view diff] no match in snippet view article find links to article

surface albedos. Microlensing is a process where relatively small and low-mass astronomical objects cause a brief small increase in the brightness of

Chi Capricorni (760 words) [view diff] no match in snippet view article find links to article

et al. (June 2010), "Sloan Low-mass Wide Pairs of Kinematically Equivalent Stars (SLoWPoKES): A Catalog of Very Wide, Low-mass Pairs", The Astronomical

NGC 6789 (231 words) [view diff] no match in snippet view article find links to article

Verheijen, Marc; Fraternali, Filippo (2014). "The triggering of starbursts in low-mass galaxies". Monthly Notices of the Royal Astronomical Society. 445 (2):

HD 89744 b (200 words) [view diff] no match in snippet view article find links to article

before 2000 Korzennik, Sylvain G.; et al. (2000). "A High-Eccentricity Low-Mass Companion to HD 89744". The Astrophysical Journal Letters. 533 (2): L147–L150

EX Lupi (1,693 words) [view diff] no match in snippet view article find links to article

constellation of Lupus. An irregular variable, it is the prototype of young, low-mass eruptive stars named EXors, with EX Lupi being this object's variable star

OGLE-TR-132b (306 words) [view diff] no match in snippet view article find links to article

star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements

Nanoelectromechanical systems (5,385 words) [view diff] case mismatch in snippet view article find links to article

derives from typical device dimensions in the nanometer range, leading to low mass, high mechanical resonance frequencies, potentially large quantum mechanical

GQ Lupi b (678 words) [view diff] no match in snippet view article find links to article

Stanimir; Cruz, Kelle L (2014). "Accretion onto Planetary Mass Companions of Low-mass Young Stars". The Astrophysical Journal Letters. 783 (1): L17. arXiv:1401

List of exoplanets discovered in 2010 (3,066 words) [view diff] no match in snippet view article find links to article

137G. doi:10.3847/1538-3881/ab6cff. S2CID 119209434. A new take on the low-mass brown dwarf companions on wide orbits in Upper-Scorpius. M. Kuzuhara, M

Döbereiner's triads (833 words) [view diff] no match in snippet view article find links to article

all the known elements could be arranged in the form of triads. For very low-mass or very high mass elements, the Döbereiner's triads are not applicable

V455 Andromedae (899 words) [view diff] case mismatch in snippet view article find links to article

has been determined. The mass of the donor star is only 0.07 M☉. This low mass makes V455 Andromedae similar to WZ Sagittae dwarf novae, which are expected

Walter Lewin (3,250 words) [view diff] no match in snippet view article find links to article

accreting neutron stars. In his search for millisecond X-ray pulsations from low-mass X-ray binaries, in 1984–85 Lewin made guest observations with the European

Mabuchi Motor (9,821 words) [view diff] case mismatch in snippet view article find links to article

lower mass and weight reduction) Power seats (including model RZ-46BWA, a low mass and high torque motor contributing to weight reduction of power seats)

Yellow hypergiant (3,525 words) [view diff] case mismatch in snippet view article find links to article

progenitors have been discovered, but they all appear to be of relatively low mass and luminosity, not hypergiants. SN 2013cu is a type IIb supernova whose

List of open clusters (1,622 words) [view diff] no match in snippet view article find links to article

S2CID 17018911. Pinfield, D. J.; et al. (July 2003). "Brown dwarfs and low-mass stars in the Pleiades and Praesepe: membership and binarity". Monthly Notices

OGLE-TR-132 (303 words) [view diff] no match in snippet view article find links to article

star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements

Serpens (11,801 words) [view diff] no match in snippet view article find links to article

of these, GX 17+2, is a low-mass X-ray binary consisting of a neutron star and, as in all low-mass X-ray binaries, a low-mass star. The system has been

AB Doradus (1,000 words) [view diff] no match in snippet view article find links to article

S2CID 16080025. Azulay, R.; et al. (June 2015), "Dynamical masses of the low-mass stellar binary AB Doradus B", Astronomy & Astrophysics, 578: 9, arXiv:1504

Macroscopic scale (1,135 words) [view diff] case mismatch in snippet view article find links to article

seem incorrect to associate "high energy" with the physics of very small, low mass–energy systems, like subatomic particles. By comparison, one gram of hydrogen

Future of an expanding universe (5,647 words) [view diff] case mismatch in snippet view article find links to article

occurs, and its lifetime as a star will properly begin. Stars of very low mass will eventually exhaust all their fusible hydrogen and then become helium

SPECULOOS (1,501 words) [view diff] no match in snippet view article find links to article

to characterise low-mass eclipsing binaries and plays an important part in the follow-up of a new class of rapidly rotating low-mass stars. SPECULOOS

List of star extremes (3,005 words) [view diff] no match in snippet view article find links to article

Le; Perrier, C. (October 2009). "Mass-radius relation of low and very low-mass stars revisited with the VLTI". Astronomy & Astrophysics. 505 (1): 205–215

Micro black hole (3,028 words) [view diff] case mismatch in snippet view article find links to article

black hole suddenly explodes. Any primordial black hole of sufficiently low mass will evaporate to near the Planck mass within the lifetime of the Universe

Ion thruster (8,769 words) [view diff] no match in snippet view article find links to article

dozens of low-power ion thrusters), use as a main propulsion engine for low-mass robotic space vehicles (such as Deep Space 1 and Dawn), and serving as

NGC 7160 (740 words) [view diff] case mismatch in snippet view article find links to article

variable circumstellar disk with mass losses (6±3)×10−11 M☉ per year. One low mass member, with spectral type K4.5 is accreting, suggesting the presence of

CT Chamaeleontis (725 words) [view diff] no match in snippet view article find links to article

CT Chamaeleontis b or as CT Chamaeleontis B, sometimes erroneously as low-mass star. The companion was proven to be most likely in the brown dwarf mass

NGC 4359 (365 words) [view diff] no match in snippet view article find links to article

-B.; Fan, X.; Wang, T.-G. (2014-01-27). "Chandraand MMT Observations of Low-Mass Black Hole Active Galactic Nuclei Accreting at Low Rates in Dwarf Galaxies"

VB 10 (1,347 words) [view diff] case mismatch in snippet view article find links to article

came as a surprise to astronomers. It had previously been assumed that low mass red dwarfs would have insignificant or nonexistent magnetic fields, which

QX Andromedae (747 words) [view diff] no match in snippet view article find links to article

at an Old Cluster: The Membership, Rotation, and Magnetic Activity of Low-mass Stars in the 1.3 Gyr Old Open Cluster NGC 752". The Astrophysical Journal

MEarth Project (370 words) [view diff] no match in snippet view article find links to article

Abstract # 1616624: The MEarth Project: An All Sky Survey of the Closest Low-mass Stars to Uncover the Very Best Terrestrial Exoplanets for Further Study"

Mu Herculis (1,303 words) [view diff] no match in snippet view article find links to article

believed to be a close binary with a low-mass stellar or a large substellar companion. This was confirmed when low-mass companion was resolved using near-infrared

DDO 44 (549 words) [view diff] no match in snippet view article find links to article

Kristine; Strader, Jay; Willman, Beth (2019). "Tidal Destruction in a Low-mass Galaxy Environment: The Discovery of Tidal Tails around DDO 44". The Astrophysical

TRAPPIST-1e (2,722 words) [view diff] no match in snippet view article find links to article

star has a mass of 0.089 M☉ – near the boundary between a brown dwarf and low-mass star – and a radius of 0.121 R☉. It has a temperature of 2,516 K (2,243 °C;

4 Equulei (681 words) [view diff] case mismatch in snippet view article find links to article

dwarf companion. Instead, the secondary may consist of a binary pair of low mass dwarfs. The visible component is an F-type main-sequence star with a stellar

Embedded cluster (384 words) [view diff] no match in snippet view article find links to article

clusters may be distributed according to initial mass function, with many low-mass stars formed for every high-mass star. Nevertheless, the high-mass stars

WZ Sagittae (896 words) [view diff] case mismatch in snippet view article find links to article

constellation Sagitta. It consists of a white dwarf primary being orbited by a low mass companion. The white dwarf is about 0.85 solar masses while the companion

HD 93385 (791 words) [view diff] no match in snippet view article find links to article

web}}: CS1 maint: postscript (link) Tokovinin, Andrei (February 2011), "Low-mass Visual Companions to Nearby G-dwarfs", The Astronomical Journal, 141 (2):

IC 348 (436 words) [view diff] no match in snippet view article find links to article

age of the IC 348 star cluster has facilitated the discovery of three low-mass brown dwarfs. As these objects cool over time, they become more detectable

Teegarden's Star b (767 words) [view diff] no match in snippet view article find links to article

percent chance of having an atmosphere.: 105–107 Teegarden’s Star is a low-mass red dwarf, with a mass of around 9 percent the mass of the Sun, and with

XTE J1739-285 (224 words) [view diff] case mismatch in snippet view article find links to article

3566. Bibcode:2007PASP..119.1108Z. doi:10.1086/522796. S2CID 15651718. Low mass X-ray binary Evidence of 1122 Hz X-Ray Burst Oscillations from the Neutron

Gliese 367 (1,026 words) [view diff] no match in snippet view article find links to article

M-dwarfs in Multiples (Min Ms) survey – I. Stellar multiplicity among low-mass stars within 15 pc★". Monthly Notices of the Royal Astronomical Society

HD 133002 (949 words) [view diff] no match in snippet view article find links to article

2006−2007 survey of nearby stars, it was discovered that HD 133002 has a low-mass common proper motion stellar companion. This object has an estimated 15%

T Tauri wind (810 words) [view diff] case mismatch in snippet view article find links to article

cloud to accrete onto the protostar, because the protostars are relatively low mass, it takes even longer to slowly contract and approach starhood. For the

HD 7449 (689 words) [view diff] no match in snippet view article find links to article

dwarf has been proposed as the cause of this trend. However, in 2015 a low-mass stellar companion (HD 7449 B) was found, which is likely the cause of the

Theta Draconis (1,044 words) [view diff] no match in snippet view article find links to article

S2CID 119511744. 21. Mazeh, Tsevi; et al. (January 2002). "Infrared Detection of Low-Mass Secondaries in Spectroscopic Binaries". The Astrophysical Journal. 564

VX Sagittarii (2,170 words) [view diff] case mismatch in snippet view article find links to article

indicates strong VO and CN. In many respects the atmosphere is similar to low mass AGB stars such as Mira variables, but with a supergiant's luminosity and

OGLE-TR-113 (385 words) [view diff] no match in snippet view article find links to article

star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements

Jupiter (16,530 words) [view diff] no match in snippet view article find links to article

Didier (June 3, 2013). "Deuterium Burning In Massive Giant Planets And Low-mass Brown Dwarfs Formed By Core-nucleated Accretion". The Astrophysical Journal

KELT-1 (736 words) [view diff] no match in snippet view article find links to article

simultaneously with a planetary companion. The star was found to be orbited by a low-mass brown dwarf or giant planet in 2012. The atmosphere of the brown dwarf

Mikko Tuomi (853 words) [view diff] no match in snippet view article find links to article

super-Earth orbiting the nearest halo red dwarf" "Bayesian search for low-mass planets around nearby M. draws. Estimates for occurrence rate based on

Teegarden's Star c (740 words) [view diff] no match in snippet view article find links to article

Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star". Astronomy & Astrophysics. 670: A84. arXiv:2301.02477. Bibcode:2023A&A

Nuclear star cluster (711 words) [view diff] no match in snippet view article find links to article

mass of most galaxies. NSCs are the central massive objects of fainter, low-mass galaxies where supermassive black holes (SMBHs) are not present or are

OGLE-2005-BLG-390L (289 words) [view diff] case mismatch in snippet view article find links to article

planet is 2.6 AU, however the orbital elements are unknown. Based on its low mass and estimated temperature of around 50 K, the planet is thought to consist

NGC 720 (1,241 words) [view diff] case mismatch in snippet view article find links to article

early-type galaxies suggest that NGC 720 may be a fossil group, despite its low mass. Further away lie the edge-on spiral galaxy NGC 681, NGC 701, and NGC 755

OGLE-TR-111 (409 words) [view diff] no match in snippet view article find links to article

object had not been measured, it was not clear that it was a true planet, low-mass red dwarf or something else. In 2004 radial velocity measurements showed

VHS J1256–1257 (1,835 words) [view diff] no match in snippet view article find links to article

Miles-Páez, Paulo A. (2021). "Detection of photometric variability in the very low-mass binary VHS J1256-1257AB using TESS and Spitzer". Astronomy & Astrophysics

Bok globule (847 words) [view diff] no match in snippet view article find links to article

Steve; Vrba, Frederick (March 1992). "Star formation in Bok globules and low-mass clouds. IV – Herbig–Haro objects in B335". Astronomy & Astrophysics. 256

Cryogenic Rare Event Search with Superconducting Thermometers (751 words) [view diff] case mismatch in snippet view article find links to article

1140/epjc/s10052-012-1971-8. S2CID 119283621. The CRESST Collaboration, Results on low mass WIMPs using an upgraded CRESST-II detector, https://arxiv.org/abs/1407

CNO cycle (2,527 words) [view diff] no match in snippet view article find links to article

formation, and evolution of low-mass stars and brown dwarfs – Energy generation". New Light on Dark Stars: Red dwarfs, low-mass stars, brown dwarfs. Springer-Praxis

2MASS J18450079–1409036 (460 words) [view diff] no match in snippet view article find links to article

Schlieder, Joshua; Bonnefoy, Mickaël; Henning, Thomas (2016), "Binaries among low-mass stars in nearby young moving groups", Astronomy & Astrophysics, 599: A70

Q2343-BX418 (337 words) [view diff] no match in snippet view article find links to article

Yuguang (May 21, 2018). "The Kinematics of Extended Lyα Emission in a Low-mass, Low-metallicity Galaxy at z = 2.3*". The Astrophysical Journal. 862 (1):

Acura ARX-02a (518 words) [view diff] case mismatch in snippet view article find links to article

to Diesel centric rules created by the ACO by exploiting the engine's low mass (low compared to larger Diesel engines). Rear tires are now fitted onto

KOI-74 (369 words) [view diff] case mismatch in snippet view article find links to article

boosting of light in the Kepler data indicates that it is likely to be a low mass white dwarf of approximately 0.22 solar masses, resulting from an earlier

NGC 4294 (1,083 words) [view diff] exact match in snippet view article find links to article

Smith, Beverly J.; Madden, Suzanne C. (1997-07-01). "Interstellar Gas in Low Mass Virgo Cluster Spiral Galaxies". The Astronomical Journal. 114: 138–146

La Silla Observatory (3,256 words) [view diff] no match in snippet view article find links to article

spectrograph with unrivalled precision and is the most successful finder of low-mass exoplanets to date. Since 2022, the 3.6 m telescope has also hosted NIRPS

NGC 4299 (1,126 words) [view diff] exact match in snippet view article find links to article

Smith, Beverly J.; Madden, Suzanne C. (1997-07-01). "Interstellar Gas in Low Mass Virgo Cluster Spiral Galaxies". The Astronomical Journal. 114: 138–146

Gibor Basri (1,314 words) [view diff] case mismatch in snippet view article find links to article

His research focused on stellar magnetic activity, star formation, and low mass stars and brown dwarfs. He was also the founding Vice Chancellor for Equity

Spectro-Polarimetric High-Contrast Exoplanet Research (2,126 words) [view diff] no match in snippet view article find links to article

young stellar associations which may also offer opportunities to detect low-mass planets; stars with known planets, in particular those with long-term residuals

List of exoplanets discovered between 2000–2009 (1,040 words) [view diff] no match in snippet view article find links to article

to have a true mass much greater than its minimum mass, and is thus a low-mass star rather than a planet. Similarly, a 2017 study showed 2MASS J21402931+1625183

HAT-P-16 (816 words) [view diff] no match in snippet view article find links to article

(2015), "Friends of Hot Jupiters. III. An Infrared Spectroscopic Search for Low-Mass Stellar Companions", The Astrophysical Journal, 814 (2): 148, arXiv:1510

Primordial black hole (6,206 words) [view diff] no match in snippet view article find links to article

would have a lifetime about equal to the age of the universe. If such low-mass black holes were created in sufficient number in the Big Bang, we should

Kepler-28 (519 words) [view diff] no match in snippet view article find links to article

Interests. New Effective Temperatures, Metallicities, Masses, and Radii of Low-mass Kepler Planet-candidate Host Stars". The Astrophysical Journal Letters

List of exoplanets discovered in 2013 (4,338 words) [view diff] no match in snippet view article find links to article

Extrasolar Planets Encyclopaedia". 1995. Retrieved 2015-11-09. PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT

R Scuti (1,177 words) [view diff] no match in snippet view article find links to article

maximum, but it is actually thought to be a highly evolved and expanded low-mass star probably no more than 10,000 times the luminosity of the sun even

HD 48265 b (224 words) [view diff] no match in snippet view article find links to article

466..443J. doi:10.1093/mnras/stw2811. Minniti, Dante; et al. (2009). "Low-Mass Companions for Five Solar-Type Stars From the Magellan Planet Search Program"

Sagittarius Window Eclipsing Extrasolar Planet Search (414 words) [view diff] no match in snippet view article find links to article

planets" (USPPs) by the search team. USPPs were discovered only around low-mass stars, suggesting that larger stars destroyed any planets orbiting so closely

Sagittarius Window Eclipsing Extrasolar Planet Search (414 words) [view diff] no match in snippet view article find links to article

planets" (USPPs) by the search team. USPPs were discovered only around low-mass stars, suggesting that larger stars destroyed any planets orbiting so closely

Mercury relay (757 words) [view diff] no match in snippet view article find links to article

the mercury-wetted relay is used instead. This combines the speed of a low-mass relay, together with the fast wetting of mercury contacts. A relay, usually

Magellan Planet Search Program (483 words) [view diff] exact match in snippet view article find links to article

175167 b HD 28185 b HD 111232 b HD 106906 b Minniti, D.; et al. (2009). "Low Mass Companions for Five Solar-Type Stars from the Magellan Planet Search Program"

Helix Nebula (1,355 words) [view diff] no match in snippet view article find links to article

Nebula is an example of a planetary nebula, formed by an intermediate to low-mass star, which sheds its outer layers near the end of its evolution. Gases

Gliese 412 (1,181 words) [view diff] no match in snippet view article find links to article

1086/381147. S2CID 8494577. Reid, I. Neill; Gizis, John E. (June 1997). "Low-Mass Binaries and the Stellar Luminosity Function". Astronomical Journal. 113:

Wolf 1069 (371 words) [view diff] no match in snippet view article find links to article

Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star". Astronomy & Astrophysics. 670: A84. arXiv:2301.02477. Bibcode:2023A&A

KOI-81 (428 words) [view diff] no match in snippet view article find links to article

of relativistic effects in the Kepler light curve suggests that it is a low-mass white dwarf of approximately 0.3 solar masses, produced by a previous stage

NGC 7013 (708 words) [view diff] no match in snippet view article find links to article

bulge-to-disk ratio and the slow rotation velocity show that NGC 7013 is a low-mass, low-density galaxy unlike the more luminous, typical lenticular galaxies

HD 102117 (595 words) [view diff] no match in snippet view article find links to article

Strasbourg. Retrieved 2021-01-28. Tinney, C. G.; et al. (2005). "Three Low-Mass Planets from the Anglo-Australian Planet Search". The Astrophysical Journal

HD 4208 b (194 words) [view diff] no match in snippet view article find links to article

Lake Managua in Nahuatl language. Vogt, Steven S.; et al. (2002). "Ten Low-Mass Companions from the Keck Precision Velocity Survey". The Astrophysical

Quattuor abhinc annos (782 words) [view diff] exact match in snippet view article find links to article

Tridentine Low Mass by a priest wearing a maniple on his left arm, Szydłowiec, Poland

List of stars in Ara (220 words) [view diff] no match in snippet view article find links to article

00.98s −49° 57′ 43.6″ K4V Low-mass X-ray binary; black hole candidate XTE J1701-462 17h 00m 58.46s −46° 11′ 08.6″ Low-mass X-ray binary Table legend:

Wolf–Rayet star (10,604 words) [view diff] no match in snippet view article find links to article

link leading to classical WN stars or the result of tidal stripping by a low-mass companion. The first three Wolf–Rayet stars to be identified, coincidentally

Habitable zone (13,731 words) [view diff] case mismatch in snippet view article find links to article

including comets, Ceres is the only one of planetary mass. A combination of low mass and an inability to mitigate evaporation and atmosphere loss against the

OGLE-TR-122 (354 words) [view diff] no match in snippet view article find links to article

Retrieved 2024-09-10. Chabrier, Gilles; Baraffe, Isabelle (2000). "Theory of Low-Mass Stars and Substellar Objects". Annual Review of Astronomy and Astrophysics

Gliese 328 (484 words) [view diff] no match in snippet view article find links to article

et al. (June 2023). "The GAPS programme at TNG. XLVI. Deep search for low-mass planets in late-dwarf systems hosting cold Jupiters". Astronomy & Astrophysics

Shuriken (1,635 words) [view diff] case mismatch in snippet view article find links to article

the eyes, face, hands, or feet.[better source needed] Shuriken, despite low mass, were capable of dealing lethal blows at short ranges. In some cases, shuriken

Peter Pan disk (2,557 words) [view diff] no match in snippet view article find links to article

Detective project discovered WISE J080822.18-644357.3 (or J0808). This low-mass star showed signs of youth, for example a strong infrared excess and active

DENIS-P J082303.1−491201 b (327 words) [view diff] no match in snippet view article find links to article

Eduardo L.; Queloz, D.; et al. (August 2013). "Astrometric orbit of a low-mass companion to an ultracool dwarf". Astronomy & Astrophysics. 556. A133.

V691 Coronae Australis (521 words) [view diff] no match in snippet view article find links to article

(April 2003). "A Spectroscopic and Photometric Study of the Eclipsing Low-mass X-Ray Binary 2A 1822-371 (V691 Coronae Australis". The Astronomical Journal

HD 114783 (539 words) [view diff] no match in snippet view article find links to article

5. Bibcode:1999MSS...C05....0H. Vogt, Steven S.; et al. (2002). "Ten Low-Mass Companions from the Keck Precision Velocity Survey". The Astrophysical

1 Boötis (469 words) [view diff] no match in snippet view article find links to article

Bibcode:1967IAUS...30...57E Hubrig, S.; et al. (June 2001), "Search for low-mass PMS companions around X-ray selected late B stars", Astronomy and Astrophysics

HD 140913 (747 words) [view diff] no match in snippet view article find links to article

masses, placing this object near the boundary between brown dwarfs and low-mass stars. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release

Gunshot wound (6,215 words) [view diff] case mismatch in snippet view article find links to article

The US military commonly uses 5.56-mm bullets, which have a relatively low mass as compared with other bullets; however, the speed of these bullets is

HAT-P-26 (983 words) [view diff] no match in snippet view article find links to article

(2015), "Friends of Hot Jupiters. III. An Infrared Spectroscopic Search for Low-Mass Stellar Companions", The Astrophysical Journal, 814 (2): 148, arXiv:1510

Astrophysics (3,300 words) [view diff] no match in snippet view article find links to article

astronomers – (includes astrophysicists) Neutrino astronomy – Observing low-mass stellar particles Timeline of gravitational physics and relativity Timeline

Messier 84 (712 words) [view diff] no match in snippet view article find links to article

ISBN 978-0-521-37079-0. Finoguenov, A.; Jones, C. (2002). "Chandra Observation of Low-Mass X-Ray Binaries in the Elliptical Galaxy M84". Astrophysical Journal. 574

Cygnus (constellation) (5,864 words) [view diff] no match in snippet view article

Zdziarski, A. A.; Mikolajewska, J.; Belczynski, K. (2012). "Cyg X-3: A low-mass black hole or a neutron star". Monthly Notices of the Royal Astronomical

Orders of magnitude (time) (1,271 words) [view diff] no match in snippet view article

pressure thereupon 300 – 600 Es (10 – 20 Ta): The estimated lifetime of low-mass stars (red dwarfs) 1021 zettasecond Zs 3 Zs (+100 Ta): The remaining time

Interacting galaxy (1,380 words) [view diff] no match in snippet view article find links to article

of early-type dwarf galaxies - the discovery of rotation in isolated, low-mass early-type galaxies". Monthly Notices of the Royal Astronomical Society

NGC 2404 (288 words) [view diff] no match in snippet view article find links to article

Kristine; Strader, Jay; Willman, Beth (2019). "Tidal Destruction in a Low-mass Galaxy Environment: The Discovery of Tidal Tails around DDO 44". The Astrophysical

Rubric (1,003 words) [view diff] exact match in snippet view article find links to article

Britannica. Vol. 23 (11th ed.). 1911. p. 810. Rubrics of the Anglican Low Mass (from 1931) Archived 2008-05-23 at the Wayback Machine Very full set of

List of stars in Mensa (138 words) [view diff] no match in snippet view article find links to article

X-ray binary LMC X-2 05h 20m 28.04s −71° 57′ 53.3″ 18.0 160000 in LMC, Low-mass X-ray binary MACHO-LMC-5 05h 16m 41.1s −70° 29′ 18″ 21.15 160000 microlensing

Luminosity (3,003 words) [view diff] case mismatch in snippet view article find links to article

2019. Delfosse, Xavier; et al. (December 2000), "Accurate masses of very low mass stars. IV. Improved mass-luminosity relations", Astronomy and Astrophysics

Protoplanetary disk (2,138 words) [view diff] no match in snippet view article find links to article

(2014). "Growth of Jupiter: Enhancement of core accretion by a voluminous low-mass envelope". Icarus. 241: 298–312. arXiv:1405.7305. Bibcode:2014Icar..241