Detached Binary Systems
Detached Binary Systems is a type of binary star system in which the two component stars are sufficiently separated in orbit that neither star fills its Roche lobe, thereby preventing mass transfer between the stars and maintaining independent stellar evolution.
142
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7.1K
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402
Authors
218
Institutions
Publications per year
2017–2026
27
Variants
Detached Binaries
Parents
142
Gas dynamics of semidetached binaries
S. H. Lubow, Frank H. Shu · The Astrophysical Journal · 1975 · 609 citations
Natural Sciences, Astronomy, Physics +17
Photometric orbits of seven detached eclipsing binaries
Daniel M. Popper, P. B. Etzel · The Astronomical Journal · 1981 · 401 citations
Natural Sciences, Astronomy, Physics +13
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218
National Astronomical Observatories
Beijing, China
12 h-index
45 publications
1.3K citations

Chinese Academy of Sciences
Beijing, China
12 h-index
48 publications
1.1K citations

Yunnan Observatories
Kunming, China
9 h-index
23 publications
656 citations
University of Chinese Academy of Sciences
Beijing, China
8 h-index
15 publications
294 citations
KU Leuven
Leuven, Belgium
7 h-index
14 publications
440 citations
Institute of Astronomy
Moscow, Russia
7 h-index
13 publications
448 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
7 h-index
10 publications
553 citations
University of Oxford
Oxford, United Kingdom
6 h-index
11 publications
330 citations
1–8 of 218
40 publications · 2.5K citations
24
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ApJ · 28 publications · 2.2K citations
22
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20 publications · 587 citations
18
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AJ · 13 publications · 723 citations
13
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Repository · 4 publications · 70 citations
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