Shock-cloud Interactions

Shock-Cloud Interactions is a physical process in astrophysics wherein the expanding shock front of a supernova remnant encounters and dynamically interacts with a dense interstellar cloud, leading to localized emission enhancements, turbulence, and potential particle acceleration.

332

Publications

18.2K

Citations

988

Authors

427

Institutions

Publications per year

2017–2026

46

Authors

988

  1. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    9 publications · 357 citations

    9

    h-index

  2. FB
    F. Bocchino

    Osservatorio Astronomico di Palermo, Italy

    7 publications · 295 citations

    7

    h-index

  3. GP
    G. Pineau des Forêts

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

    6 publications · 400 citations

    6

    h-index

  4. SO
    S. Orlando

    Osservatorio Astronomico di Palermo, Italy

    6 publications · 277 citations

    6

    h-index

  5. JC
    J. C. Raymond

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 688 citations

    6

    h-index

1–5 of 988

Venues

  1. The Astrophysical Journal

    ApJ · 107 publications · 8.4K citations

    47

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    42 publications · 1.5K citations

    24

    h-index

  3. Astronomy and Astrophysics

    25 publications · 1.6K citations

    21

    h-index

  4. The Astrophysical Journal Letters

    9 publications · 414 citations

    9

    h-index

  5. The Astronomical Journal

    AJ · 9 publications · 299 citations

    9

    h-index

1–5