Disk-wind Interactions

Disk-Wind Interactions is a theoretical framework in astrophysical accretion theory that describes the mutual influence between accretion disk dynamics and magnetically or thermally driven outflows, distinguishing it from isolated disk or wind models by explicitly coupling angular momentum transport, mass loss, and energy exchange processes between the rotating disk and the emerging wind.

552

Publications

42.9K

Citations

1.1K

Authors

531

Institutions

Publications per year

2017–2026

148

Variants

Disk-wind Interaction

Authors

1.1K

  1. DP
    Daniel Proga

    University of Nevada, Las Vegas, United States

    19 publications · 2.5K citations

    18

    h-index

  2. RE
    Ralph E. Pudritz

    McMaster University, Canada

    15 publications · 1.9K citations

    15

    h-index

  3. TR
    T. R. Kallman

    Goddard Space Flight Center, United States

    13 publications · 2.2K citations

    13

    h-index

  4. SC
    S. Cabrit

    Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France

    13 publications · 698 citations

    12

    h-index

  5. JM
    J. M. Mïller

    University of Michigan, United States

    11 publications · 952 citations

    11

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 240 publications · 24.8K citations

    82

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    70 publications · 3.9K citations

    36

    h-index

  3. Astronomy and Astrophysics

    67 publications · 3.6K citations

    33

    h-index

  4. The Astrophysical Journal Letters

    28 publications · 2.2K citations

    21

    h-index

  5. 13

    h-index

1–5