Binary Stellar Evolution
Binary Stellar Evolution is a theoretical framework in astrophysics that models the coeval development and mutual interactions of two gravitationally bound stars, distinguishing itself from single-star evolution by incorporating mass transfer, tidal forces, and orbital dynamics as fundamental drivers of stellar lifecycle changes.
856
Publications
71.7K
Citations
2.9K
Authors
745
Institutions
Publications per year
2017–2026
348
856
Binary Interaction Dominates the Evolution of Massive Stars
H. Sana, S. E. de Mink, A. de Koter et al. · Science · 2012 · 2.1K citations · Full text
Natural Sciences, Astronomy, Physics +16
Binary Evolution in Stellar Dynamics
Douglas C. Heggie · Monthly Notices of the Royal Astronomical Society · 1975 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +16
Evolutionary Processes in Close Binary Systems
B. Paczyński · Annual Review of Astronomy and Astrophysics · 1971 · 1.1K citations
Natural Sciences, Astronomy, Physics +17
1–5 of 856
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745
Northwestern University
Evanston, United States
37 h-index
156 publications
16.8K citations

Radboud University Nijmegen
Nijmegen, The Netherlands
35 h-index
78 publications
7.3K citations
University of Bonn
Bonn, Germany
33 h-index
109 publications
17.5K citations

University of Amsterdam
Amsterdam, The Netherlands
32 h-index
92 publications
9.1K citations
KU Leuven
Leuven, Belgium
32 h-index
109 publications
6.5K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
30 h-index
87 publications
8.4K citations
Institute of Astronomy
Moscow, Russia
29 h-index
75 publications
7.5K citations
University of Cambridge
Cambridge, United Kingdom
27 h-index
48 publications
7.5K citations
1–8 of 745
ApJ · 237 publications · 21.7K citations
78
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221 publications · 18.3K citations
73
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112 publications · 7.1K citations
47
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35 publications · 2.5K citations
26
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16 publications · 778 citations
15
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