Gas Disk Dynamics

Gas Disk Dynamics is the study of the motion and evolution of gaseous material within circumstellar disks, distinguished by its focus on the physical processes governing angular momentum transport, viscosity, and pressure gradients in rotating astrophysical disks.

461

Publications

37.3K

Citations

1.1K

Authors

475

Institutions

Publications per year

2017–2026

118

Authors

1.1K

  1. BV
    B. Vollmer

    Observatoire astronomique de Strasbourg, France

    8 publications · 706 citations

    8

    h-index

  2. RT
    Richard Teague

    Center for Astrophysics Harvard & Smithsonian, United States

    8 publications · 548 citations

    8

    h-index

  3. KW
    Keiichi Wada

    National Astronomical Observatory of Japan, Japan

    8 publications · 352 citations

    8

    h-index

  4. SI
    Shigeru Ida

    Tokyo Institute of Technology, Japan

    8 publications · 655 citations

    8

    h-index

  5. AH
    Asao Habe

    Hokkaido University, Japan

    6 publications · 189 citations

    6

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 199 publications · 17.3K citations

    67

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    55 publications · 3.8K citations

    35

    h-index

  3. Astronomy and Astrophysics

    47 publications · 2.3K citations

    27

    h-index

  4. The Astronomical Journal

    AJ · 26 publications · 3.5K citations

    22

    h-index

  5. The Astrophysical Journal Letters

    19 publications · 901 citations

    17

    h-index

1–5