Accretion Onto Compact Objects
Accretion Onto Compact Objects is a theoretical framework in astrophysics that describes the dynamical and radiative processes by which matter gravitationally bound to a compact object—such as a black hole, neutron star, or white dwarf—loses angular momentum and energy to spiral inward and accumulate onto the object’s surface or event horizon, distinguishing it from general accretion phenomena by the dominance of extreme gravitational fields, relativistic effects, and high-energy emission mechanisms.
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2017–2026
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491
Cracking of self-gravitating compact objects
L. Herrera · Physics Letters A · 1992 · 985 citations
Natural Sciences, Astronomy, Physics +12
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Center for Astrophysics Harvard & Smithsonian, United States
7 publications · 1.6K citations
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
59 publications
8.3K citations

Centre National de la Recherche Scientifique
Paris, France
18 h-index
68 publications
8.5K citations
California Institute of Technology
Pasadena, United States
14 h-index
25 publications
2.4K citations
University of Maryland, College Park
College Park, United States
13 h-index
17 publications
1.4K citations
Université Paris Cité
Paris, France
13 h-index
46 publications
5K citations
University of Southampton
Southampton, United Kingdom
13 h-index
26 publications
1.4K citations

University of Amsterdam
Amsterdam, The Netherlands
13 h-index
31 publications
1.7K citations

Silesian University in Opava
Opava, Czechia
13 h-index
23 publications
1.1K citations
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ApJ · 135 publications · 11.4K citations
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92 publications · 8.1K citations
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35 publications · 1.7K citations
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PRD · 17 publications · 751 citations
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