Core-collapse Supernovae

Core-Collapse Supernovae is a theoretical astrophysical phenomenon denoting the catastrophic gravitational collapse of the iron core of a massive star, leading to a violent explosion that emits multi-messenger signals including neutrinos, gravitational waves, and electromagnetic radiation.

2.1K

Publications

185.3K

Citations

9.8K

Authors

1.3K

Institutions

Publications per year

2017–2026

746

Authors

9.8K

  1. HJ
    Hans‐Thomas Janka

    Max Planck Institute for Astrophysics, Germany

    60 publications · 11.3K citations

    47

    h-index

  2. AB
    Adam Burrows

    University of Arizona, United States

    54 publications · 5.2K citations

    43

    h-index

  3. KK
    Kei Kotake

    National Astronomical Observatory of Japan, Japan

    53 publications · 4.1K citations

    38

    h-index

  4. TT
    Tomoya Takiwaki

    National Astronomical Observatory of Japan, Japan

    44 publications · 3.5K citations

    35

    h-index

  5. SY
    Shoichi Yamada

    Waseda University, Japan

    45 publications · 2.6K citations

    33

    h-index

1–5 of 9.8K

Venues

  1. The Astrophysical Journal

    ApJ · 607 publications · 65.4K citations

    134

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    293 publications · 22.1K citations

    84

    h-index

  3. Astronomy and Astrophysics

    123 publications · 11.7K citations

    59

    h-index

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

    PRD · 118 publications · 5.5K citations

    46

    h-index

  5. The Astrophysical Journal Letters

    72 publications · 6K citations

    42

    h-index

1–5