Nucleosynthesis Yields

Nucleosynthesis Yields is a theoretical construct in astrophysics that quantifies the total mass of each chemical element produced and ejected into the interstellar medium by a stellar population over its lifetime, distinguished by its role in modeling the chemical enrichment of galaxies.

355

Publications

40K

Citations

948

Authors

380

Institutions

Publications per year

2017–2026

83

Authors

948

  1. KN
    K. Nomoto

    The University of Tokyo, Japan

    12 publications · 3.4K citations

    12

    h-index

  2. AH
    Alexander Heger

    Monash University, Australia

    11 publications · 1.2K citations

    11

    h-index

  3. FT
    F.‐K. Thielemann

    University of Basel, Switzerland

    11 publications · 1.2K citations

    11

    h-index

  4. CK
    Chiaki Kobayashi

    University of Hertfordshire, United Kingdom

    10 publications · 3.6K citations

    10

    h-index

  5. KA
    Keith A. Olive

    University of Minnesota, United States

    9 publications · 2K citations

    9

    h-index

1–5 of 948

Venues

  1. The Astrophysical Journal

    ApJ · 89 publications · 8.4K citations

    45

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    38 publications · 3.4K citations

    30

    h-index

  3. Astronomy and Astrophysics

    17 publications · 1.4K citations

    16

    h-index

  4. Nuclear Physics A

    13 publications · 1.1K citations

    11

    h-index

  5. Earth and Planetary Science Letters

    11 publications · 2.7K citations

    11

    h-index

1–5