Supernova-driven Turbulence

Supernova-Driven Turbulence is a theoretical construct within astrophysics that denotes the large-scale, chaotic interstellar gas motions sustained primarily by the cumulative mechanical energy input from recurrent supernova explosions in the diffuse interstellar medium.

120

Publications

8.8K

Citations

262

Authors

209

Institutions

Publications per year

2017–2026

42

Authors

262

  1. MM
    Mordecai‐Mark Mac Low

    American Museum of Natural History, United States

    11 publications · 1.2K citations

    11

    h-index

  2. FA
    Frederick A. Gent

    Newcastle University, United Kingdom

    4 publications · 120 citations

    4

    h-index

  3. RT
    Romain Teyssier

    University of Zurich, Switzerland

    4 publications · 478 citations

    4

    h-index

  4. OG
    Oliver Gressel

    Leibniz Institute for Astrophysics Potsdam, Germany

    4 publications · 271 citations

    4

    h-index

  5. GL
    Greg L. Bryan

    Columbia University, United States

    3 publications · 352 citations

    3

    h-index

1–5 of 262

Venues

  1. The Astrophysical Journal

    ApJ · 38 publications · 3.5K citations

    29

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    25 publications · 1.4K citations

    21

    h-index

  3. Astronomy and Astrophysics

    14 publications · 1.2K citations

    14

    h-index

  4. The Astrophysical Journal Letters

    4 publications · 314 citations

    4

    h-index

  5. 3

    h-index

1–5