Disk Accretion Processes

Disk Accretion Processes is a theoretical framework in astrophysics that describes the mechanisms by which matter gradually spirals inward through a circumstellar disk toward a central protostellar object due to angular momentum transport and viscous dissipation.

641

Publications

53.3K

Citations

1.4K

Authors

603

Institutions

Publications per year

2017–2026

147

Authors

1.4K

  1. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    23 publications · 4.2K citations

    22

    h-index

  2. LT
    L. Testi

    Arcetri Astrophysical Observatory, Italy

    14 publications · 1.4K citations

    14

    h-index

  3. SJ
    Scott J. Kenyon

    Smithsonian Astrophysical Observatory, United States

    13 publications · 2.5K citations

    13

    h-index

  4. NC
    Nuria Calvet

    University of Michigan, United States

    12 publications · 1.7K citations

    12

    h-index

  5. DN
    D. N. C. Lin

    University of California, Santa Cruz, United States

    8 publications · 498 citations

    8

    h-index

1–5 of 1.4K

Venues

  1. The Astrophysical Journal

    ApJ · 253 publications · 28K citations

    88

    h-index

  2. Astronomy and Astrophysics

    80 publications · 5.6K citations

    43

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    48 publications · 4.4K citations

    33

    h-index

  4. The Astrophysical Journal Letters

    16 publications · 668 citations

    16

    h-index

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

    Repository · 15 publications · 898 citations

    14

    h-index

1–5