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

Authors

964

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    13 publications · 1.8K citations

    13

    h-index

  2. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 1.4K citations

    12

    h-index

  3. JP
    Jeremiah P. Ostriker

    Princeton University, United States

    11 publications · 543 citations

    11

    h-index

  4. MC
    Mitchell C. Begelman

    Joint Institute for Laboratory Astrophysics, United States

    9 publications · 2.5K citations

    9

    h-index

  5. KI
    Kohei Inayoshi

    Peking University, China

    8 publications · 480 citations

    8

    h-index

1–5 of 964

Venues

  1. The Astrophysical Journal

    ApJ · 157 publications · 11.7K citations

    62

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    115 publications · 9.6K citations

    44

    h-index

  3. Astronomy and Astrophysics

    38 publications · 1.4K citations

    22

    h-index

  4. The Astrophysical Journal Letters

    13 publications · 856 citations

    12

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 12 publications · 1.1K citations

    12

    h-index

1–5