Accretion Disk Physics

Accretion Disk Physics is a theoretical framework within high-energy astrophysics that describes the dynamical, radiative, and magnetohydrodynamic processes governing matter as it spirals inward through a rotating disk around a compact gravitational object.

4K

Publications

296.7K

Citations

7.1K

Authors

1.5K

Institutions

Publications per year

2017–2026

760

Authors

7.1K

  1. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    39 publications · 7.7K citations

    33

    h-index

  2. MA
    M. A. Abramowicz

    Nicolaus Copernicus Astronomical Center, Poland

    36 publications · 5K citations

    29

    h-index

  3. JC
    J. C. B. Papaloizou

    Queen Mary University of London, United Kingdom

    38 publications · 4.9K citations

    28

    h-index

  4. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    38 publications · 3.9K citations

    27

    h-index

  5. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    32 publications · 4.9K citations

    27

    h-index

1–5 of 7.1K

Venues

  1. The Astrophysical Journal

    ApJ · 1.7K publications · 146.2K citations

    171

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    544 publications · 41.2K citations

    99

    h-index

  3. Astronomy and Astrophysics

    361 publications · 19.5K citations

    70

    h-index

  4. The Astrophysical Journal Letters

    134 publications · 6K citations

    43

    h-index

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

    Repository · 87 publications · 4.9K citations

    37

    h-index

1–5