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Find link is a tool written by Edward Betts.Longer titles found: Common envelope jets supernova (view), Post common envelope binary (view)
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Kepler-451
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J19383260+4603591 and abbreviated to 2M1938+4603) is an eclipsing post-common envelope binary star system that comprises two stars, a pulsating subdwarf BEnvelope (music) (697 words) [view diff] exact match in snippet view article
synthesizers, samplers, and other electronic musical instruments. The most common envelope generator is controlled with four parameters: attack, decay, sustainW Ursae Majoris variable (494 words) [view diff] exact match in snippet view article find links to article
stars are close binaries of spectral types F, G, or K that share a common envelope of material and are thus in contact with one another. They are termedNGC 545 (719 words) [view diff] exact match in snippet view article find links to article
equally bright NGC 547, which lies 0.5 arcminutes away. They share a common envelope, however, despite their close position, no tidal features like tailsNGC 547 (742 words) [view diff] exact match in snippet view article find links to article
equally bright NGC 545, which lies 0.5 arcminutes away. They share a common envelope, however, despite their close position, no tidal features like tailsV471 Tauri (700 words) [view diff] exact match in snippet view article find links to article
spectral type D2; and a K-type main sequence star (K2 V), together a post-common envelope binary. There are variations in the timing of the eclipses that wereVW Leonis Minoris (630 words) [view diff] exact match in snippet view article find links to article
A-type W Ursae Majoris eclipsing binary, where the two stars share a common envelope. The eclipse of the primary causes the magnitude of the system to dropWolf–Rayet nebula (449 words) [view diff] exact match in snippet view article find links to article
(2022). "3D mapping of the Wolf–Rayet nebula M 1-67: Clues for post-common envelope evolution in massive stars". Monthly Notices of the Royal AstronomicalNSVS 14256825 (1,054 words) [view diff] exact match in snippet view article find links to article
S. (2018). "The quest for stable circumbinary companions to post-common envelope SDB eclipsing binaries. Does the observational evidence support theirQS Virginis (461 words) [view diff] case mismatch in snippet view article find links to article
V. S.; et al. (2010). "Orbital Period Variations in Eclipsing Post Common Envelope Binaries". Monthly Notices of the Royal Astronomical Society. 407 (4):NGC 5910 (675 words) [view diff] exact match in snippet view article find links to article
and MCG+04-36-036. The other galaxies appear to be embedded within a common envelope that belongs to NGC 5910. NGC 5910 appears to lie near the HerculesAisle (company) (489 words) [view diff] no match in snippet view article
were a liner-on-top style cloth menstrual pad as opposed to the more common "envelope" style. The pads have two parts; a Pad Base which snaps around theMario Livio (1,717 words) [view diff] exact match in snippet view article find links to article
a supernova explosion. He was one of the pioneers in the study of common envelope evolution of binary stars, and he applied the results to the shapingNGC 5189 (509 words) [view diff] no match in snippet view article find links to article
McBride, Vanessa (1 April 2015). "A radial velocity survey for post-common-envelope Wolf–Rayet central stars of planetary nebulae: first results and discoveryNY Virginis (1,066 words) [view diff] exact match in snippet view article find links to article
von Harrach, S. (August 2022). "Eclipse timing variations in post-common envelope binaries: Are they a reliable indicator of circumbinary companionsKOI-256 (760 words) [view diff] case mismatch in snippet view article find links to article
"Characterizing the Cool KOIs. V. KOI-256: A Mutually Eclipsing Post-common Envelope Binary". The Astrophysical Journal. 767 (2). 111. arXiv:1304.1165.NGC 2293 (596 words) [view diff] exact match in snippet view article find links to article
away from NGC 2292 lies NGC 2293. Both galaxies appear to share a common envelope and a complete ring of neutral hydrogen gas (HI) has been found toTriple-twin (370 words) [view diff] exact match in snippet view article find links to article
triple-twin contained two dissimilar, directly coupled triodes in a common envelope. To maximize power yield, the output triode was intended to be positivelyPolar (star) (1,307 words) [view diff] exact match in snippet view article
Gomez-Moran, A.; Schreiber, M. R.; Gänsicke, B. T. (2009-04-29). "Post common envelope binaries from the SDSS. VI. SDSS J120615.73+510047.0: a new low accretionAstroid (1,157 words) [view diff] exact match in snippet view article find links to article
Astroid x2⁄3 + y2⁄3 = r2⁄3 as the common envelope of a family of ellipses of equation (x⁄a)2 + (y⁄b)2 = r2, where a + b = 1.NGC 2346 (658 words) [view diff] no match in snippet view article find links to article
Boffin, Henri M. J.; Van Winckel, Hans (February 2019). "On the post-common-envelope central star of the planetary nebula NGC 2346". Monthly Notices ofDY Centauri (1,014 words) [view diff] exact match in snippet view article find links to article
interacted in the past when the primary had larger dimensions, forming a common envelope. Stars of R Coronae Borealis variable (RCB) type are believed to beM1-67 (773 words) [view diff] exact match in snippet view article find links to article
(2022). "3D mapping of the Wolf–Rayet nebula M 1-67: Clues for post-common envelope evolution in massive stars". Monthly Notices of the Royal AstronomicalOlivier Chesneau (206 words) [view diff] exact match in snippet view article find links to article
hypergiant HR 5171 A: Resolving a massive interacting binary in the common envelope phase". Astronomy & Astrophysics. 563: A71. arXiv:1401.2628. Bibcode:2014A&ADiscoglossus pictus (734 words) [view diff] exact match in snippet view article find links to article
1.0 to 1.5 mm; the gelatinous envelope is 3.7 mm. The eggs have no common envelope and form a loose mass on the water surface or may sink to the bottomPSR J0337+1715 (904 words) [view diff] exact match in snippet view article find links to article
other stars and creating a common envelope between it and said star. The engulfed star was slowed down from the common envelope gas, transferring its orbitalSmall Magellanic Cloud (2,694 words) [view diff] exact match in snippet view article find links to article
bridge of gas is a star-forming site. The Magellanic Clouds have a common envelope of neutral hydrogen, indicating they have been gravitationally boundLarge Magellanic Cloud (3,894 words) [view diff] exact match in snippet view article find links to article
tidal interaction between the galaxies. The Magellanic Clouds have a common envelope of neutral hydrogen, indicating that they have been gravitationallySynthesizer (5,231 words) [view diff] exact match in snippet view article find links to article
such as amplitude (volume), filters (frequencies), or pitch. The most common envelope is the ADSR (attack, decay, sustain, release) envelope: Attack is theFrosty Leo Nebula (806 words) [view diff] exact match in snippet view article find links to article
bipolar outflow being directed by a precessing disc or a precessing common envelope binary. Forveille et al. 1987 dubbed IRAS 09371+1212 as the "FrostyCNO cycle (2,600 words) [view diff] no match in snippet view article find links to article
chemical evolution of the secondary stars in close binaries, arising from common-envelope evolution and nova outbursts". Monthly Notices of the Royal AstronomicalOphlitaspongia papilla (399 words) [view diff] exact match in snippet view article find links to article
populations. The result may be equivalent to cross-fertilisation within a common envelope and result in an enlarged gene pool and the efficient production ofLie sphere geometry (3,959 words) [view diff] exact match in snippet view article find links to article
natural description of Dupin cyclides. These are characterized as the common envelope of two one parameter families of spheres S(s) and T(t), where S andBe–white dwarf X-ray binary system (1,093 words) [view diff] exact match in snippet view article find links to article
to spin up the secondary to Be star velocities without triggering common envelope evolution. Tidal synchronization mechanisms explain the observed lackMensa (constellation) (4,071 words) [view diff] exact match in snippet view article
Majoris variable; the two components are so close that they share a common envelope of stellar material. The larger star has been calculated to be 1.86VZ Piscium (1,332 words) [view diff] case mismatch in snippet view article find links to article
(September 1989), "UU-Cancri and VZ-Piscium, Contact Systems Before the Common Envelope Phase?", Astrophysics and Space Science, 159 (1): 67–83, Bibcode:1989Ap&SSBartazoon (227 words) [view diff] exact match in snippet view article find links to article
microgametogenesis with production of a small number of gametes within a common envelope along with the macrogamete. Sporogony occurs in a single step. SporocystList of exoplanet firsts (2,980 words) [view diff] exact match in snippet view article find links to article
Hermes, J. J. (2010). "Two planets orbiting the recently formed post-common envelope binary NN Serpentis". Astronomy and Astrophysics. 521: L60. arXiv:1010List of exoplanets discovered in 2012 (4,190 words) [view diff] exact match in snippet view article find links to article
Hessman, F. V.; Deller, J. (2012). "The quest for companions to post-common envelope binaries. III. A reexamination of HW Virginis". Astronomy & AstrophysicsIK Pegasi (5,203 words) [view diff] exact match in snippet view article find links to article
stars in IK Pegasi, so during this time period the two stars shared a common envelope. As a result, the outer atmosphere of IK Pegasi A may have receivedFirst observation of gravitational waves (7,592 words) [view diff] exact match in snippet view article find links to article
like GW would be prevented. The survival of such binaries, through common envelope phases of high rotation in massive progenitor stars, may be necessaryAbell 63 (1,250 words) [view diff] no match in snippet view article find links to article
nebula nuclei UU Sagitte and V477 Lyrae: oversized secondaries in post-common-envelope binaries", Monthly Notices of the Royal Astronomical Society, 391 (2):List of exoplanet extremes (8,406 words) [view diff] exact match in snippet view article find links to article
von Harrach, S. (August 2022). "Eclipse timing variations in post-common envelope binaries: Are they a reliable indicator of circumbinary companionsGlossary of astronomy (19,104 words) [view diff] exact match in snippet view article find links to article
atmosphere; or another name for the stellar atmosphere itself. 2. The common envelope of gases encompassing a binary star system. stellar evolution stellarList of exoplanets discovered in 2018 (6,527 words) [view diff] case mismatch in snippet view article find links to article
; Wang, Q.-S.; Voloshina, Irina (2018). "DE CVn: An Eclipsing Post-common Envelope Binary with a Circumbinary Disk and a Giant Planet". The AstrophysicalOY Arae (726 words) [view diff] case mismatch in snippet view article find links to article
1093/mnras/227.1.23. Sparks, Warren M.; Sion, Edward M. (2021). "Nova-produced Common Envelope: Source of the Nonsolar Abundances and an Additional Frictional AngularAbell 30 (1,888 words) [view diff] exact match in snippet view article find links to article
G; Tafoya, D; Chu, Y-H; Ramos-Larios, G; Sabin, L (6 July 2022). "Common envelope evolution in born-again planetary nebulae – Shaping the H-deficient