Close Binary Orbital Evolution is a theoretical framework in astrophysics that models the dynamical changes in the orbital parameters of two gravitationally bound stars in a close binary system due to energy and angular momentum exchange mechanisms such as mass transfer, tidal interactions, and gravitational radiation.
139
Publications
7.5K
Citations
272
Authors
148
Institutions
Publications per year
2017–2026
15
Parents
Publications
139
1–5 of 139
Authors
272
- CD
7
h-index
- JP
7
h-index
- SQ
5
h-index
- TM
4
h-index
- RF
3
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1–5 of 272
Institutions
148
Vrije Universiteit Brussel
Brussels, Belgium
8 h-index
18 publications
782 citations
Chinese Academy of Sciences
Beijing, China
6 h-index
8 publications
182 citations
National Astronomical Observatories
Beijing, China
6 h-index
8 publications
223 citations
University of Cambridge
Cambridge, United Kingdom
5 h-index
6 publications
1.2K citations
Yunnan Observatories
Kunming, China
5 h-index
7 publications
162 citations
University of St Andrews
St Andrews, United Kingdom
4 h-index
4 publications
582 citations
Observatoire de Paris
Paris, France
4 h-index
5 publications
220 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
6 publications
838 citations
1–8 of 148
Venues
- The Astrophysical Journal
ApJ · 24 publications · 2.5K citations
21
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- Monthly Notices of the Royal Astronomical Society
22 publications · 1.6K citations
17
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- Astrophysics and Space Science
18 publications · 401 citations
13
h-index
- Astronomy and Astrophysics
7 publications · 253 citations
7
h-index
- The Astronomical Journal
AJ · 6 publications · 141 citations
5
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1–5