Supernova-driven Gas

Supernova-Driven Gas is a dynamical state of interstellar gas characterized by bulk motion and thermal energization resulting directly from the mechanical energy input and shock propagation of nearby supernova explosions.

368

Publications

30.3K

Citations

1.1K

Authors

438

Institutions

Publications per year

2017–2026

59

Authors

1.1K

  1. RA
    Roger A. Chevalier

    University of Virginia, United States

    10 publications · 1.1K citations

    10

    h-index

  2. JS
    Joseph Silk

    University of Oxford, United Kingdom

    9 publications · 2.5K citations

    9

    h-index

  3. SC
    Simon C. O. Glover

    Heidelberg University, Germany

    8 publications · 924 citations

    8

    h-index

  4. RS
    Ralf S. Klessen

    Heidelberg University, Germany

    7 publications · 902 citations

    7

    h-index

  5. RW
    Richard Wünsch

    Czech Academy of Sciences, Astronomical Institute, Czechia

    7 publications · 948 citations

    7

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 147 publications · 13.3K citations

    63

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    69 publications · 6.8K citations

    43

    h-index

  3. Astronomy and Astrophysics

    19 publications · 1K citations

    16

    h-index

  4. The Astrophysical Journal Letters

    17 publications · 843 citations

    14

    h-index

  5. Nature

    11 publications · 2.4K citations

    11

    h-index

1–5