Supernova Yields

Supernova Yields is a theoretical construct in astrophysics that quantifies the mass of newly synthesized elements ejected into the interstellar medium by a supernova explosion, distinguishing it from other nucleosynthetic outputs through its specific association with explosive stellar death.

169

Publications

14.9K

Citations

374

Authors

230

Institutions

Publications per year

2017–2026

44

Authors

374

  1. AH
    Alexander Heger

    Monash University, Australia

    8 publications · 978 citations

    8

    h-index

  2. KN
    K. Nomoto

    The University of Tokyo, Japan

    8 publications · 2.4K citations

    8

    h-index

  3. FT
    F.‐K. Thielemann

    University of Basel, Switzerland

    7 publications · 680 citations

    7

    h-index

  4. CL
    Chris L. Fryer

    Los Alamos National Laboratory, United States

    6 publications · 355 citations

    6

    h-index

  5. NT
    Nozomu Tominaga

    The University of Tokyo, Japan

    6 publications · 2.2K citations

    6

    h-index

1–5 of 374

Venues

  1. The Astrophysical Journal

    ApJ · 66 publications · 6.7K citations

    38

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    24 publications · 1.7K citations

    20

    h-index

  3. Astronomy and Astrophysics

    16 publications · 2.1K citations

    16

    h-index

  4. CERN Document Server (European Organization for Nuclear Research)

    Repository · 5 publications · 387 citations

    5

    h-index

  5. The Astrophysical Journal Letters

    4 publications · 433 citations

    4

    h-index

1–5