Galactic Chemical Evolution

Galactic Chemical Evolution is a theoretical framework in astrophysics that describes the progressive change in chemical composition of baryonic matter within galaxies over cosmic time due to stellar nucleosynthesis, supernova explosions, and galactic-scale gas dynamics.

1.3K

Publications

109K

Citations

3.1K

Authors

790

Institutions

Publications per year

2017–2026

278

Authors

3.1K

  1. FM
    F. Matteuccí

    Trieste Astronomical Observatory, Italy

    91 publications · 7.1K citations

    46

    h-index

  2. CC
    C. Chiappini

    Leibniz Institute for Astrophysics Potsdam, Germany

    32 publications · 4.9K citations

    29

    h-index

  3. TC
    Timothy C. Beers

    Michigan State University, United States

    27 publications · 5.4K citations

    25

    h-index

  4. DR
    D. Romano

    Trieste Astronomical Observatory, Italy

    24 publications · 1.9K citations

    22

    h-index

  5. ES
    E. Spitoni

    Trieste Astronomical Observatory, Italy

    25 publications · 1.3K citations

    22

    h-index

1–5 of 3.1K

Venues

  1. The Astrophysical Journal

    ApJ · 379 publications · 38.9K citations

    104

    h-index

  2. Astronomy and Astrophysics

    227 publications · 17.8K citations

    71

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    211 publications · 15.8K citations

    68

    h-index

  4. The Astronomical Journal

    AJ · 44 publications · 3.7K citations

    28

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 43 publications · 1.7K citations

    25

    h-index

1–5