Accretion Disk Spectra

Accretion Disk Spectra is a theoretical construct in astrophysics that characterizes the electromagnetic radiation emitted across various wavelengths due to viscous dissipation of gravitational energy in differentially rotating plasma surrounding a compact gravitational source.

1K

Publications

77.8K

Citations

2.2K

Authors

701

Institutions

Publications per year

2017–2026

172

Authors

2.2K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    43 publications · 4.9K citations

    34

    h-index

  2. JM
    J. M. Mïller

    University of Michigan, United States

    37 publications · 3.2K citations

    30

    h-index

  3. CS
    C. S. Reynolds

    University of Maryland, College Park, United States

    23 publications · 2.8K citations

    23

    h-index

  4. KH
    K. Horne

    University of St Andrews, United Kingdom

    20 publications · 1.7K citations

    18

    h-index

  5. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    20 publications · 1.8K citations

    17

    h-index

1–5 of 2.2K

Venues

  1. The Astrophysical Journal

    ApJ · 467 publications · 38.6K citations

    101

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    175 publications · 11.8K citations

    60

    h-index

  3. Astronomy and Astrophysics

    101 publications · 5.7K citations

    40

    h-index

  4. The Astronomical Journal

    AJ · 25 publications · 2.3K citations

    20

    h-index

  5. The Astrophysical Journal Letters

    21 publications · 1.8K citations

    19

    h-index

1–5