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Find link is a tool written by Edward Betts.searching for warm Dust 38 found (47 total)
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Wreath Nebula
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new stars are being born. The green ring is made of tiny particles of warm dust whose composition is very similar to smog. The red cloud in the middleExozodiacal dust (914 words) [view diff] case mismatch in snippet view article find links to article
Around 1 in 100 stars in the nearby solar systems shows a high content of warm dust that is around 1000 times greater than the average dust emission in theNGC 2232 (558 words) [view diff] case mismatch in snippet view article find links to article
display an infrared excess at a wavelength of 8μm that is suggestive of warm dust, while the A-type star HD 45435 displays a strong excess at 24μm. TheSigma Andromedae (973 words) [view diff] case mismatch in snippet view article find links to article
photometric variations and is used as an ubvy standard star. A debris disk of warm dust around this star has been detected by Spitzer Space Telescope. A modelHD 113766 (1,054 words) [view diff] case mismatch in snippet view article find links to article
the 4.4 L☉ HD 113766 A. The group found at least a Mars' mass worth of warm dust in particles of size 10 m or less, and very likely as much as a few EarthSN 1987A (5,023 words) [view diff] case mismatch in snippet view article find links to article
is a typical representative of its class then the derived mass of the warm dust formed in the debris of core collapse supernovae is not sufficient toEta Corvi (1,858 words) [view diff] case mismatch in snippet view article find links to article
The warm dust is very primitive, and definitely not from an asteroidal parent body. A large amount, at least 3 x 1019 kg, of 0.1 – 1000 μm warm dust isBD+20°307 (895 words) [view diff] exact match in snippet view article find links to article
Thompson, Maggie A.; et al. (12 April 2019). "Studying the Evolution of Warm Dust Encircling BD+20 307 Using SOFIA". The Astrophysical Journal. 875 (1):Giant-impact hypothesis (6,849 words) [view diff] case mismatch in snippet view article find links to article
(~12 My old) star HD 172555 in the Beta Pictoris moving group. A belt of warm dust in a zone between 0.25AU and 2AU from the young star HD 23514 in the PleiadesNGC 5363 (991 words) [view diff] exact match in snippet view article find links to article
Fazio, G. G.; Willner, S. P. (September 2004). "Spatial Distribution of Warm Dust in Early-Type Galaxies". The Astrophysical Journal Supplement Series.IRAS 00500+6713 (885 words) [view diff] case mismatch in snippet view article find links to article
extreme stellar wind, surrounded by a nebula packed with hot gas and warm dust. The star represents a new kind of X-ray source. It exhibits record-breakingEpsilon Eridani (11,490 words) [view diff] case mismatch in snippet view article find links to article
disc consisting of a Kuiper belt analogue at 70 au from the star and warm dust between about 3 au and 20 au from the star. The gap in the debris discHD 107146 (909 words) [view diff] case mismatch in snippet view article find links to article
(2018), "A gap in the planetesimal disc around HD 107146 and asymmetric warm dust emission revealed by ALMA", Monthly Notices of the Royal AstronomicalTau1 Aquarii (679 words) [view diff] exact match in snippet view article find links to article
1051/0004-6361:20000451, S2CID 425754. Morales, Farisa Y.; et al. (April 2011), "Common Warm Dust Temperatures Around Main-sequence Stars" (PDF), The Astrophysical JournalHD 316285 (1,230 words) [view diff] case mismatch in snippet view article find links to article
an unusually high emission at infrared wavelengths due to surrounding warm dust. In 1961, HD 316285 was catalogued as planetary nebula Bl3-11, althoughLSPM J0207+3331 (920 words) [view diff] exact match in snippet view article find links to article
Collaboration; The Disk Detective Collaboration (2019). "A 3 Gyr White Dwarf with Warm Dust Discovered via the Backyard Worlds: Planet 9 Citizen Science Project"Frost line (astrophysics) (1,584 words) [view diff] case mismatch in snippet view article
planet formation inside their orbit. By analysing the temperature of warm dust found around some 90 stars, they concluded that the dust (and thereforePi Arae (703 words) [view diff] exact match in snippet view article find links to article
retrieved 2017-09-26. Morales, Farisa Y.; et al. (April 2011), "Common Warm Dust Temperatures Around Main-sequence Stars" (PDF), The Astrophysical JournalNGC 300 (1,941 words) [view diff] exact match in snippet view article find links to article
"ATEL 2660: Optical and Near-IR Follow-up of SN 2010da: Evidence for Warm Dust". Astronomers Telegram. 2010-06-04. Retrieved 2010-06-11. "ClassificationRho Aquilae (862 words) [view diff] exact match in snippet view article find links to article
1086/318269, S2CID 18154947. Morales, Farisa Y.; et al. (April 2011), "Common Warm Dust Temperatures Around Main-sequence Stars", The Astrophysical Journal LettersEpsilon Eridani b (1,743 words) [view diff] case mismatch in snippet view article find links to article
1051/0004-6361/200811609. Reidemeister, Martin; et al. (2010). "The cold origin of the warm dust around epsilon Eridani". Astronomy & Astrophysics. 527: A57. arXiv:1011Stephenson 2 DFK 49 (1,457 words) [view diff] case mismatch in snippet view article find links to article
be an underestimate, because it does not include excess radiation from warm dust. Davies (2007) estimated its temperature of 3,920 K, but with an uncertaintyRR Telescopii (1,734 words) [view diff] case mismatch in snippet view article find links to article
mutual orbit with a white dwarf, with substantial amounts of hot gas and warm dust around the two stars. The red giant is frequently referred to as a MiraTabby's Star (9,031 words) [view diff] case mismatch in snippet view article find links to article
Optical Telescope in Spain. A massive collision scenario would create warm dust that glows in infrared wavelengths, but there is no observed excess infraredCosmic dust (5,828 words) [view diff] case mismatch in snippet view article find links to article
Astronomers used the James Webb Space Telescope to image the warm dust around a nearby young star, Fomalhaut, in order to study the first asteroid beltHypergiant (4,477 words) [view diff] exact match in snippet view article find links to article
1051/0004-6361/201118440. S2CID 17900583. Robberto, M.; Herbst, T. M. (1998). "Warm Dust around Blue Hypergiants: Mid-Infrared Imaging of the Luminous Blue VariableWhite dwarf (17,798 words) [view diff] exact match in snippet view article find links to article
Jacqueline K.; Rees, Jon M. (19 February 2019). "A 3 Gyr White Dwarf with Warm Dust Discovered via the Backyard Worlds: Planet 9 Citizen Science Project"Hubble Deep Field (3,866 words) [view diff] case mismatch in snippet view article find links to article
cirrus, the diffuse, wispy infrared emission believed to be caused by warm dust grains in cool clouds of hydrogen gas (H I regions). These criteria restrictedMartian polar ice caps (5,156 words) [view diff] case mismatch in snippet view article find links to article
formation of the spiders says that sunlight heats dust grains in the ice. The warm dust grains settle by melting through the ice while the holes are annealedType II supernova (4,792 words) [view diff] case mismatch in snippet view article find links to article
which leads to an increased temperature of the cirumstellar dust. This warm dust can be observed as a brightening in the mid-infrared light. If the circumstellarMessier 87 (9,550 words) [view diff] case mismatch in snippet view article find links to article
than 25 μm. Normally, this may be an indication of thermal emission by warm dust. In the case of M87, the emission can be fully explained by synchrotronProxima Centauri (10,171 words) [view diff] case mismatch in snippet view article find links to article
about 1.2 arcseconds from the star. There was a hint at an additional warm dust belt at a distance of 0.4 AU from the star. However, upon further analysisHR 8799 (4,217 words) [view diff] case mismatch in snippet view article find links to article
around HR 8799. Three components of the debris disk were distinguished: Warm dust (T ≈ 150 K) orbiting within the innermost planet (e). The inner and outerSerpens–Aquila Rift (1,551 words) [view diff] case mismatch in snippet view article find links to article
The molecular cloud at these wavelengths is traced by emission from warm dust in the clouds, allowing the structure of the clouds to be probed. WaveletList of Ingenuity flights (2,773 words) [view diff] case mismatch in snippet view article find links to article
percent on Ingenuity's solar array, which charges its batteries, and warm dust lowered the surrounding air density by seven percent, which could haveJ1000+1242 (890 words) [view diff] case mismatch in snippet view article find links to article
both sides of its narrow-line region concealed by a torus of gas and warm dust, or a circumnuclear ring. A bright emission line region is also foundList of exoplanets and planetary debris around white dwarfs (5,035 words) [view diff] exact match in snippet view article find links to article
Collaboration; The Disk Detective Collaboration (2019). "A 3 Gyr White Dwarf with Warm Dust Discovered via the Backyard Worlds: Planet 9 Citizen Science Project"List of resolved circumstellar disks (7,061 words) [view diff] case mismatch in snippet view article find links to article
(2018-10-01). "A gap in the planetesimal disc around HD 107146 and asymmetric warm dust emission revealed by ALMA". Monthly Notices of the Royal Astronomical