Stellar Nucleosynthesis

Stellar Nucleosynthesis is an astrophysical process of nucleosynthesis in which chemical elements are formed and transmuted through nuclear fusion and associated nuclear reactions in the interiors and explosive endpoints of stars, thereby producing most elements heavier than those created in Big Bang nucleosynthesis.

2.2K

Publications

201.7K

Citations

3.7K

Authors

1K

Institutions

Publications per year

2017–2026

426

Authors

3.7K

  1. RG
    R. Gallino

    University of Turin, Italy

    63 publications · 11.9K citations

    47

    h-index

  2. FT
    F.‐K. Thielemann

    University of Basel, Switzerland

    60 publications · 11.2K citations

    44

    h-index

  3. MW
    M. Wiescher

    University of Notre Dame, United States

    54 publications · 5.3K citations

    36

    h-index

  4. SE
    S. E. Woosley

    University of California, Santa Cruz, United States

    43 publications · 14K citations

    35

    h-index

  5. KN
    K. Nomoto

    The University of Tokyo, Japan

    44 publications · 8.8K citations

    33

    h-index

1–5 of 3.7K

Venues

  1. The Astrophysical Journal

    ApJ · 751 publications · 75.2K citations

    140

    h-index

  2. Astronomy and Astrophysics

    183 publications · 14.3K citations

    68

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    177 publications · 15.1K citations

    64

    h-index

  4. The Astrophysical Journal Letters

    64 publications · 5.3K citations

    38

    h-index

  5. The Astrophysical Journal Supplement Series

    42 publications · 11.4K citations

    36

    h-index

1–5