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Common Envelope Evolution of Massive Binary Stars
Annual Review of Astronomy and Astrophysics, 2000▪ Abstract The common envelope phase of binary star evolution plays an essential role in the formation of short period systems containing a compact object. In this process, significant mass and angular momentum are lost, transforming a wide progenitor system into a close remnant binary. The pathways leading to this phase and the outcomes are described.
Eric Sandquist
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The Formation of Common-Envelope, Pre-Main-Sequence Binary Stars
Astrophysics and Space Science Library, 1999Recent observational investigations of the frequency of occurrence of premain-sequence binary stars have reinforced earlier suspicions that “binary formation is the primary branch of the star-formation process” (Mathieu 1994). As Bodenheimer et al. (1993) have reviewed, a number of different theories have been proposed to explain the preponderance of ...
J E Tohline
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Post-common-envelope binary central stars of Planetary Nebulae in the OGLE-IV survey [PDF]
, 2016 Planetary Nebulae (PNe) are defined as the ionized shells of circumstellar gas ejected through an intense stellar wind at the end of the star's life. PNe come in different shapes, from spherical to highly complex, non-spherical shapes. Mass loss in AGB stars is presumed as the shaping mechanism but how it results in different PNe morphologies is still ...
Hlabathe, Michael
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Common envelopes in binary star evolution
Publications of the Astronomical Society of the Pacific, 1993The characteristics of many close, evolved binaries can be understood most easily if there exists some agency that can abstract angular momentum or mass, or both, from the precursor system. Close binaries may be defined as systems in which at least one of the components has filled or will fill its Roche lobe and attempt to transfer matter to its ...
Icko, Jr. Iben, Mario Livio
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AGB stars in binaries and the common envelope interaction
Proceedings of the International Astronomical Union, 2018AbstractOne may argue that, today, proceedings articles are not useful. Results belong in refereed papers and even reviews are best in publications that are long enough to do justice to the topic reviewed. In this short review, reflecting a presentation that was given at the IAU343 symposium, Why Galaxies Care about AGB Stars, I have therefore ...
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Simulating the onset of grazing envelope evolution of binary stars
Monthly Notices of the Royal Astronomical Society: Letters, 2017Sagiv Shiber, Amit Kashi, Noam Soker
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Presupernova Evolution of Massive Single and Binary Stars
Annual Review of Astronomy and Astrophysics, 2012Norbert Langer
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Envelope density pattern around wide binary AGB stars: a dynamical model
Astronomy and Astrophysics, 2007J H He
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