Binary Accretion
Binary Accretion is a theoretical framework in astrophysical accretion processes that specifically describes the transfer and accumulation of matter from one stellar component to another within a binary star system, distinguished by the gravitational interaction and orbital dynamics between the two compact or evolving companions.
206
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12.1K
Citations
411
Authors
254
Institutions
Publications per year
2017–2026
64
Parents
206
A model of accretion disks in close binaries
B. Paczyński · The Astrophysical Journal · 1977 · 413 citations
Natural Sciences, Astronomy, Physics +15
Accretion during the Merger of Supermassive Black Holes
The Astrophysical Journal · 2002 · 406 citations · Full text
Natural Sciences, Astronomy, Physics +17
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254
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
12 h-index
29 publications
2.6K citations
University of Cambridge
Cambridge, United Kingdom
11 h-index
19 publications
538 citations

Space Telescope Science Institute
Baltimore, United States
8 h-index
10 publications
772 citations

Kyoto University
Kyoto, Japan
8 h-index
17 publications
725 citations
Rochester Institute of Technology
Rochester, United States
7 h-index
15 publications
1.6K citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
8 publications
730 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
6 h-index
7 publications
478 citations

Pennsylvania State University
State College, United States
6 h-index
13 publications
382 citations
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ApJ · 48 publications · 4.3K citations
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59 publications · 3.5K citations
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15 publications · 508 citations
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9 publications · 602 citations
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6 publications · 384 citations
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