Accretion Disk Emission

Accretion Disk Emission is a radiative astrophysical phenomenon arising from the release of gravitational potential energy in an accretion disk, wherein matter spiraling toward a compact object emits electromagnetic radiation, predominantly in the X-ray band, due to viscous heating in the disk's inner, high-temperature regions.

1.1K

Publications

90.1K

Citations

3.4K

Authors

903

Institutions

Publications per year

2017–2026

222

Authors

3.4K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    32 publications · 3.7K citations

    27

    h-index

  2. NC
    Nuria Calvet

    University of Michigan, United States

    26 publications · 7K citations

    22

    h-index

  3. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    26 publications · 5.2K citations

    22

    h-index

  4. JM
    J. M. Mïller

    University of Michigan, United States

    23 publications · 2K citations

    20

    h-index

  5. CS
    C. S. Reynolds

    University of Maryland, College Park, United States

    18 publications · 2.6K citations

    17

    h-index

1–5 of 3.4K

Venues

  1. The Astrophysical Journal

    ApJ · 483 publications · 44.8K citations

    103

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    165 publications · 10.3K citations

    55

    h-index

  3. Astronomy and Astrophysics

    93 publications · 4.4K citations

    36

    h-index

  4. The Astrophysical Journal Letters

    36 publications · 1.3K citations

    22

    h-index

  5. The Astronomical Journal

    AJ · 24 publications · 2.8K citations

    20

    h-index

1–5