Core-collapse Supernova Remnants

Core-Collapse Supernova Remnants is a subclass of supernova remnants originating specifically from the gravitational collapse of massive stars (>8 M☉) that undergo core-collapse supernovae, distinguished by their association with neutron stars or black holes, enrichment of heavy elements synthesized during the explosion, and characteristic expansion dynamics driven by the ejected stellar envelope interacting with the surrounding interstellar medium.

970

Publications

73.3K

Citations

4.2K

Authors

938

Institutions

Publications per year

2017–2026

232

Authors

4.2K

  1. WP
    William P. Blair

    Johns Hopkins University, United States

    21 publications · 1.2K citations

    20

    h-index

  2. NS
    Noam Soker

    Technion – Israel Institute of Technology, Israel

    21 publications · 579 citations

    16

    h-index

  3. CL
    Chris L. Fryer

    Los Alamos National Laboratory, United States

    16 publications · 1.9K citations

    16

    h-index

  4. KS
    Knox S. Long

    Space Telescope Science Institute, United States

    17 publications · 898 citations

    15

    h-index

  5. YC
    You‐Hua Chu

    University of Illinois Urbana-Champaign, United States

    15 publications · 708 citations

    15

    h-index

1–5 of 4.2K

Venues

  1. The Astrophysical Journal

    ApJ · 358 publications · 28.2K citations

    86

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    122 publications · 7.4K citations

    50

    h-index

  3. Astronomy and Astrophysics

    58 publications · 3.6K citations

    35

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 31 publications · 1.7K citations

    23

    h-index

  5. The Astrophysical Journal Letters

    30 publications · 1.9K citations

    23

    h-index

1–5