Supernova Remnants

Supernova Remnants is an astrophysical structure consisting of a diffuse, expanding nebula of stellar ejecta and swept-up interstellar medium bounded by shock fronts that is created by a supernova explosion and serves as a major site of high-energy (X-ray and gamma-ray) emission and dynamical and chemical feedback into the interstellar medium.

5.8K

Publications

368.1K

Citations

12.6K

Authors

1.7K

Institutions

Publications per year

2017–2026

1.1K

Authors

12.6K

  1. AV
    A. V. Filippenko

    University of California, Berkeley, United States

    94 publications · 11.6K citations

    54

    h-index

  2. RA
    Roger A. Chevalier

    University of Virginia, United States

    87 publications · 10K citations

    52

    h-index

  3. RK
    R. Kirshner

    Center for Astrophysics Harvard & Smithsonian, United States

    68 publications · 5.8K citations

    47

    h-index

  4. JP
    John P. Hughes

    Rutgers, The State University of New Jersey, United States

    83 publications · 6K citations

    46

    h-index

  5. SP
    Stephen P. Reynolds

    North Carolina State University, United States

    78 publications · 5.8K citations

    45

    h-index

1–5 of 12.6K

Venues

  1. The Astrophysical Journal

    ApJ · 2.2K publications · 150.1K citations

    162

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    850 publications · 48.5K citations

    101

    h-index

  3. Nature

    150 publications · 28.4K citations

    77

    h-index

  4. Astronomy and Astrophysics

    464 publications · 23.1K citations

    76

    h-index

  5. The Astrophysical Journal Letters

    194 publications · 10.9K citations

    58

    h-index

1–5