Radiative Accretion Processes
Radiative Accretion Processes is a theoretical framework in astrophysics that describes the mechanisms by which gravitational energy released during matter inflow onto compact objects is converted into electromagnetic radiation through dissipative processes in the accretion flow.
472
Publications
34.6K
Citations
964
Authors
459
Institutions
Publications per year
2017–2026
99
Parents
472
<i>Accretion Power in Astrophysics</i>
Juhan Frank, A. R. King, D. J. Raine et al. · Physics Today · 1986 · 1.3K citations
Natural Sciences, Astronomy, Physics +17
Sources of Gravitational Radiation
Patrick J. McCarthy · Physics Bulletin · 1980 · 749 citations
Natural Sciences, Astronomy, Physics +17
1–5 of 472
964
13
h-index
Center for Astrophysics Harvard & Smithsonian, United States
12 publications · 1.4K citations
12
h-index
11
h-index
Joint Institute for Laboratory Astrophysics, United States
9 publications · 2.5K citations
9
h-index
8
h-index
1–5 of 964
459
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
30 h-index
81 publications
7.9K citations
Princeton University
Princeton, United States
22 h-index
26 publications
2.2K citations

Centre National de la Recherche Scientifique
Paris, France
20 h-index
74 publications
3.3K citations
University of Maryland, College Park
College Park, United States
18 h-index
26 publications
3.3K citations
Harvard University
Cambridge, United States
17 h-index
40 publications
4.9K citations

Kyoto University
Kyoto, Japan
16 h-index
27 publications
2.4K citations

Shanghai Astronomical Observatory
Shanghai, China
16 h-index
37 publications
1.4K citations
Institute of Astronomy
Moscow, Russia
15 h-index
24 publications
3.5K citations
1–8 of 459
ApJ · 157 publications · 11.7K citations
62
h-index
115 publications · 9.6K citations
44
h-index
38 publications · 1.4K citations
22
h-index
13 publications · 856 citations
12
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Repository · 12 publications · 1.1K citations
12
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1–5