Semi-Detached Binary Systems is a class of binary star systems in which one star fills its Roche lobe and transfers mass to its companion, while the other remains within its Roche lobe, thereby distinguishing it from detached and contact binaries.
99
Publications
5.2K
Citations
318
Authors
142
Institutions
Publications per year
2017–2026
10
Variants
Semi-detached Binaries
Parents
Publications
99
Gas dynamics of semidetached binaries
S. H. Lubow, Frank H. Shu · The Astrophysical Journal · 1975 · 609 citations
Natural Sciences, Astronomy, Physics +17
1–5 of 99
Authors
318
- RW
6
h-index
- MK
4
h-index
- JK
4
h-index
- MK
4
h-index
- AU
4
h-index
1–5 of 318
Institutions
142
National Astronomical Observatories
Beijing, China
10 h-index
33 publications
762 citations
Chinese Academy of Sciences
Beijing, China
10 h-index
60 publications
1.3K citations
Institute of Astronomy
Moscow, Russia
8 h-index
16 publications
1.1K citations
University of Warsaw
Warsaw, Poland
8 h-index
23 publications
1.2K citations
University of Chinese Academy of Sciences
Beijing, China
7 h-index
23 publications
648 citations
KU Leuven
Leuven, Belgium
6 h-index
16 publications
429 citations
Yunnan Observatories
Kunming, China
6 h-index
32 publications
856 citations
Royal Observatory of Belgium
Brussels, Belgium
5 h-index
10 publications
245 citations
1–8 of 142
Venues
- Monthly Notices of the Royal Astronomical Society
22 publications · 1.9K citations
17
h-index
- Astronomy and Astrophysics
15 publications · 562 citations
13
h-index
- The Astronomical Journal
AJ · 10 publications · 322 citations
10
h-index
- The Astrophysical Journal
ApJ · 11 publications · 933 citations
10
h-index
- Astronomy and Astrophysics Supplement Series
6 publications · 193 citations
6
h-index
1–5