Detached Binary Stars
Detached Binary Stars is a type of binary star system in which the two component stars are sufficiently separated by distance to evolve independently without significant gravitational interaction or mass transfer between them.
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5.4K
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212
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135
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2017–2026
11
Variants
Detached Binary Star Systems
Parents
84
Gas dynamics of semidetached binaries
S. H. Lubow, Frank H. Shu · The Astrophysical Journal · 1975 · 609 citations
Natural Sciences, Astronomy, Physics +17
Mass transfer between double white dwarfs
T. R. Marsh, G. Nelemans, D. Steeghs · Monthly Notices of the Royal Astronomical Society · 2004 · 299 citations · Full text
Natural Sciences, Astronomy, Physics +14
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135

University of Concepción
Concepción, Chile
6 h-index
24 publications
1.7K citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
15 publications
892 citations

Keele University
Newcastle-under-Lyme, United Kingdom
6 h-index
13 publications
433 citations
Observatoire de la Côte d’Azur
Nice, France
5 h-index
8 publications
640 citations
University of Southampton
Southampton, United Kingdom
5 h-index
6 publications
747 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
5 h-index
5 publications
350 citations

University of Warsaw
Warsaw, Poland
5 h-index
17 publications
636 citations
Université Paris Cité
Paris, France
5 h-index
7 publications
252 citations
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ApJ · 31 publications · 2.2K citations
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16 publications · 1.6K citations
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8 publications · 309 citations
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AJ · 4 publications · 130 citations
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Repository · 2 publications · 63 citations
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