Accretion Disk Simulations

Accretion Disk Simulations is a computational methodology within numerical astrophysics that specifically models the dynamical, radiative, and magnetic processes in rotating gaseous structures around compact celestial objects by numerically solving the equations of hydrodynamics or magnetohydrodynamics under general relativistic or Newtonian gravitational frameworks.

463

Publications

40.8K

Citations

700

Authors

360

Institutions

Publications per year

2017–2026

93

Authors

700

  1. JF
    John F. Hawley

    University of Virginia, United States

    14 publications · 3.1K citations

    13

    h-index

  2. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 2.5K citations

    12

    h-index

  3. HK
    Hubert Klahr

    Max Planck Institute for Astronomy, Germany

    12 publications · 1.3K citations

    12

    h-index

  4. JM
    James M. Stone

    Princeton University, United States

    11 publications · 1.3K citations

    11

    h-index

  5. JH
    Julian H. Krolik

    Johns Hopkins University, United States

    11 publications · 1.2K citations

    11

    h-index

1–5 of 700

Venues

  1. The Astrophysical Journal

    ApJ · 174 publications · 19.4K citations

    68

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    123 publications · 10.5K citations

    54

    h-index

  3. Astronomy and Astrophysics

    39 publications · 2.2K citations

    25

    h-index

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

    Repository · 10 publications · 986 citations

    10

    h-index

  5. 10

    h-index

1–5