Disk-binary Interaction
Disk–Binary Interaction is a theoretical construct in astrophysics that describes the dynamical and gravitational coupling between a circumstellar or circumbinary accretion disk and a binary star system, distinguishing it from isolated star–disk interactions by incorporating mutual feedback in mass transfer, angular momentum exchange, and orbital evolution during binary star formation.
235
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15.8K
Citations
555
Authors
305
Institutions
Publications per year
2017–2026
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
19 h-index
44 publications
4K citations

Centre National de la Recherche Scientifique
Paris, France
16 h-index
57 publications
2.7K citations

Université Grenoble Alpes
Saint-Martin-d'Hères, France
13 h-index
31 publications
1.3K citations
California Institute of Technology
Pasadena, United States
12 h-index
21 publications
1.6K citations
University of Cambridge
Cambridge, United Kingdom
11 h-index
21 publications
1.3K citations
Leiden University
Leiden, The Netherlands
11 h-index
13 publications
774 citations
University of Chile
Santiago, Chile
10 h-index
17 publications
1.2K citations

Space Telescope Science Institute
Baltimore, United States
10 h-index
17 publications
1.4K citations
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ApJ · 72 publications · 7.5K citations
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Repository · 8 publications · 175 citations
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