Accretion Disk Winds

Accretion Disk Winds is a physical phenomenon in accretion physics characterized by the outflow of ionized gas or plasma from the surface layers of an accretion disk, driven by radiation pressure, magnetic forces, or thermal effects, thereby removing mass, angular momentum, and energy from the disk system.

271

Publications

21K

Citations

565

Authors

358

Institutions

Publications per year

2017–2026

84

Authors

565

  1. DP
    Daniel Proga

    University of Nevada, Las Vegas, United States

    12 publications · 1.8K citations

    12

    h-index

  2. RE
    Ralph E. Pudritz

    McMaster University, Canada

    11 publications · 1.2K citations

    11

    h-index

  3. CK
    C. Knigge

    University of Southampton, United Kingdom

    9 publications · 399 citations

    9

    h-index

  4. JF
    Jun Fükue

    Osaka Kyoiku University, Japan

    8 publications · 313 citations

    8

    h-index

  5. TR
    T. R. Kallman

    Goddard Space Flight Center, United States

    8 publications · 1.5K citations

    8

    h-index

1–5 of 565

Venues

  1. The Astrophysical Journal

    ApJ · 121 publications · 12.1K citations

    56

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    44 publications · 2.2K citations

    24

    h-index

  3. Astronomy and Astrophysics

    19 publications · 1.5K citations

    18

    h-index

  4. The Astrophysical Journal Letters

    16 publications · 678 citations

    15

    h-index

  5. 12

    h-index

1–5