Stellar Metallicities

Stellar Metallicities is a quantitative astrophysical construct that measures the abundance fraction of chemical elements heavier than helium in a star relative to hydrogen, serving as a key diagnostic for stellar nucleosynthetic history and galactic chemical evolution.

5.3K

Publications

438.1K

Citations

8K

Authors

1.4K

Institutions

Publications per year

2017–2026

1.2K

Authors

8K

  1. TC
    Timothy C. Beers

    Michigan State University, United States

    165 publications · 22.8K citations

    78

    h-index

  2. JE
    John E. Norris

    Australian National University, Australia

    80 publications · 9.4K citations

    55

    h-index

  3. VH
    V. Hill

    Centre National de la Recherche Scientifique, France

    81 publications · 11K citations

    54

    h-index

  4. MA
    M. Asplund

    Australian National University, Australia

    83 publications · 10.6K citations

    54

    h-index

  5. NC
    N. C. Santos

    Universidade do Porto, Portugal

    75 publications · 9.3K citations

    50

    h-index

1–5 of 8K

Venues

  1. The Astrophysical Journal

    ApJ · 1.5K publications · 138.4K citations

    167

    h-index

  2. Astronomy and Astrophysics

    900 publications · 76.7K citations

    134

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    953 publications · 71.2K citations

    120

    h-index

  4. The Astronomical Journal

    AJ · 420 publications · 40.4K citations

    106

    h-index

  5. The Astrophysical Journal Letters

    147 publications · 9.5K citations

    56

    h-index

1–5