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The Formation of Common-Envelope, Pre-Main-Sequence Binary Stars
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, J. E. Cazes, H. S. Cohl
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The impact of recombination energy on simulations of the common-envelope binary interaction
Monthly Notices of the Royal Astronomical Society, 2020Thomas Reichardt +2 more
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Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
Annual Review of Astronomy and Astrophysics, 2014Nathan Smith
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Formation of the widest binary stars from dynamical unfolding of triple systems
Nature, 2012Bo Reipurth
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Binary stars as the key to understanding planetary nebulae
Nature Astronomy, 2017David Jones, Henri Boffin
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Binary stars in the new millennium
Progress in Particle and Nuclear PhysicsXuefei Chen, Zheng-Wei Liu, Zhan-Wen Han
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The evolution and explosion of massive binary stars and Type Ib-Ic-IIb-IIL supernovae
Physics Reports, 1995exaly