Supernova Remnant Evolution

Supernova Remnant Evolution is a theoretical framework that describes the temporal development and structural changes of supernova remnants as they interact with the interstellar medium, distinguishing itself from related astrophysical processes by focusing on the hydrodynamical, thermal, and radiative phases following stellar explosion.

1.1K

Publications

70.6K

Citations

2.3K

Authors

748

Institutions

Publications per year

2017–2026

198

Authors

2.3K

  1. RA
    Roger A. Chevalier

    University of Virginia, United States

    23 publications · 2.6K citations

    20

    h-index

  2. FB
    F. Bocchino

    Osservatorio Astronomico di Palermo, Italy

    22 publications · 1.2K citations

    18

    h-index

  3. SP
    Stephen P. Reynolds

    North Carolina State University, United States

    20 publications · 2.3K citations

    18

    h-index

  4. JP
    John P. Hughes

    Rutgers, The State University of New Jersey, United States

    19 publications · 1.9K citations

    17

    h-index

  5. PS
    Patrick Slane

    Center for Astrophysics Harvard & Smithsonian, United States

    20 publications · 1.5K citations

    17

    h-index

1–5 of 2.3K

Venues

  1. The Astrophysical Journal

    ApJ · 416 publications · 31.3K citations

    86

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    148 publications · 7.9K citations

    44

    h-index

  3. Astronomy and Astrophysics

    99 publications · 5.3K citations

    44

    h-index

  4. Nature

    27 publications · 3.1K citations

    23

    h-index

  5. The Astrophysical Journal Letters

    27 publications · 1.6K citations

    22

    h-index

1–5