Supernova Progenitors

Supernova Progenitors is the class of stars or stellar systems in specific evolutionary states whose physical properties (such as mass, composition, and, where relevant, binary configuration) render them the immediate precursors of supernova explosions.

4.3K

Publications

368K

Citations

8.6K

Authors

1.5K

Institutions

Publications per year

2017–2026

1.1K

Authors

8.6K

  1. AV
    A. V. Filippenko

    University of California, Berkeley, United States

    180 publications · 21.9K citations

    85

    h-index

  2. AG
    A. Gal‐Yam

    Weizmann Institute of Science, Israel

    143 publications · 16.6K citations

    74

    h-index

  3. PA
    P. A. Mazzali

    Max Planck Institute for Astrophysics, Germany

    130 publications · 16.9K citations

    71

    h-index

  4. KN
    K. Nomoto

    The University of Tokyo, Japan

    108 publications · 20.6K citations

    65

    h-index

  5. SJ
    S. J. Smartt

    Queen's University Belfast, United Kingdom

    99 publications · 12.5K citations

    64

    h-index

1–5 of 8.6K

Venues

  1. The Astrophysical Journal

    ApJ · 1.3K publications · 132.2K citations

    175

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    709 publications · 51.3K citations

    117

    h-index

  3. Astronomy and Astrophysics

    358 publications · 26.5K citations

    88

    h-index

  4. Nature

    172 publications · 31.4K citations

    83

    h-index

  5. The Astrophysical Journal Letters

    191 publications · 14.9K citations

    71

    h-index

1–5