Interstellar Shock Heating

Interstellar Shock Heating is a physical process in astrophysics whereby the kinetic energy of a supernova blast wave is transferred to the surrounding interstellar medium through shock fronts, resulting in a rapid increase in thermal energy and temperature of the ambient gas.

195

Publications

16.5K

Citations

614

Authors

290

Institutions

Publications per year

2017–2026

31

Authors

614

  1. CF
    Christopher F. McKee

    University of California, Berkeley, United States

    4 publications · 934 citations

    4

    h-index

  2. GP
    G. Pineau des Forêts

    Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France

    4 publications · 205 citations

    4

    h-index

  3. AG
    A. Gusdorf

    Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France

    4 publications · 353 citations

    4

    h-index

  4. PG
    P. Guillard

    Centre National de la Recherche Scientifique, France

    4 publications · 219 citations

    4

    h-index

  5. RA
    Roger A. Chevalier

    University of Virginia, United States

    4 publications · 388 citations

    4

    h-index

1–5 of 614

Venues

  1. The Astrophysical Journal

    ApJ · 81 publications · 5.1K citations

    43

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    22 publications · 1.1K citations

    19

    h-index

  3. Astronomy and Astrophysics

    12 publications · 669 citations

    12

    h-index

  4. The Astronomical Journal

    AJ · 6 publications · 216 citations

    6

    h-index

  5. arXiv (Cornell University)

    Repository · 5 publications · 78 citations

    5

    h-index

1–5