Disk Stability

Disk Stability is a theoretical construct in galactic dynamics that characterizes the resistance of a galactic disk to gravitational perturbations, distinguishing it from other stability analyses by specifically addressing the interplay between rotational support, velocity dispersion, and self-gravity in thin, rotating stellar systems.

395

Publications

39.3K

Citations

672

Authors

349

Institutions

Publications per year

2017–2026

53

Authors

672

  1. JA
    J. A. Sellwood

    Rutgers, The State University of New Jersey, United States

    8 publications · 782 citations

    8

    h-index

  2. EG
    Evgeny Griv

    Ben-Gurion University of the Negev, Israel

    7 publications · 164 citations

    7

    h-index

  3. AB
    Alessandro B. Romeo

    Chalmers University of Technology, Sweden

    6 publications · 448 citations

    6

    h-index

  4. AD
    Avishai Dekel

    Hebrew University of Jerusalem, Israel

    6 publications · 1.4K citations

    6

    h-index

  5. PS
    Patricio S. Letelier

    Universidade Estadual de Campinas (UNICAMP), Brazil

    6 publications · 173 citations

    6

    h-index

1–5 of 672

Venues

  1. The Astrophysical Journal

    ApJ · 134 publications · 21.7K citations

    60

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    89 publications · 9.4K citations

    40

    h-index

  3. Astronomy and Astrophysics

    20 publications · 1K citations

    15

    h-index

  4. 6

    h-index

  5. The Astrophysical Journal Letters

    6 publications · 427 citations

    6

    h-index

1–5