Compact Object Accretion
Compact Object Accretion is a high-energy astrophysical process in which matter gravitationally bound to a compact object—such as a black hole, neutron star, or white dwarf—loses angular momentum and spirals inward through an accretion disk, converting gravitational potential energy into electromagnetic radiation and particle acceleration.
258
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17.6K
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850
Authors
371
Institutions
Publications per year
2017–2026
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
16 h-index
51 publications
9.1K citations

University of Amsterdam
Amsterdam, The Netherlands
13 h-index
26 publications
2.5K citations
University of Southampton
Southampton, United Kingdom
13 h-index
26 publications
819 citations
Goddard Space Flight Center
Greenbelt, United States
12 h-index
26 publications
3K citations
Max Planck Institute for Astrophysics
Garching, Germany
12 h-index
17 publications
2.5K citations
California Institute of Technology
Pasadena, United States
11 h-index
19 publications
1.2K citations

Centre National de la Recherche Scientifique
Paris, France
10 h-index
27 publications
1.4K citations
National Institute for Astrophysics
Rome, Italy
9 h-index
31 publications
1.1K citations
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ApJ · 64 publications · 5K citations
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73 publications · 5.8K citations
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37 publications · 1.7K citations
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Repository · 7 publications · 115 citations
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Repository · 7 publications · 147 citations
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