Binary Population Synthesis
Binary Population Synthesis is a computational modeling framework that simulates the statistical evolution of binary star systems within a galactic population by integrating physical processes such as mass transfer, stellar winds, and mergers to predict observable properties and occurrence rates.
370
Publications
26.9K
Citations
598
Authors
328
Institutions
Publications per year
2017–2026
170
Parents
370
The origin of subdwarf B stars - II
Zhanwen Han, Philipp Podsiadlowski, P. F. L. Maxted et al. · Monthly Notices of the Royal Astronomical Society · 2003 · 693 citations · Full text
Natural Sciences, Astronomy, Physics +17
U. Heber · Annual Review of Astronomy and Astrophysics · 2009 · 473 citations
Natural Sciences, Astronomy, Physics +17
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328
Northwestern University
Evanston, United States
32 h-index
98 publications
11.2K citations
National Astronomical Observatories
Beijing, China
27 h-index
68 publications
9K citations

Chinese Academy of Sciences
Beijing, China
27 h-index
100 publications
8K citations

Monash University
Melbourne, Australia
27 h-index
76 publications
6.2K citations

Radboud University Nijmegen
Nijmegen, The Netherlands
25 h-index
62 publications
5.2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
61 publications
5K citations

University of Birmingham
Birmingham, United Kingdom
24 h-index
83 publications
8.1K citations

Yunnan Observatories
Kunming, China
21 h-index
79 publications
3K citations
1–8 of 328
126 publications · 10K citations
55
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ApJ · 71 publications · 4.5K citations
40
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51 publications · 4.1K citations
34
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14 publications · 566 citations
14
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Repository · 10 publications · 874 citations
10
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