Mass-metallicity Relation

The Mass-Metallicity Relation is an empirical astrophysical correlation that describes the observed trend wherein the gas-phase metallicity of a star-forming galaxy increases with its stellar mass, reflecting the interplay between star formation, chemical enrichment, and galactic-scale feedback processes.

1.8K

Publications

157.5K

Citations

4.2K

Authors

881

Institutions

Publications per year

2017–2026

522

Variants

Mass-metallicity RelationshipMzr

Authors

4.2K

  1. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    26 publications · 2.4K citations

    24

    h-index

  2. DA
    Duncan A. Forbes

    Swinburne University of Technology, Australia

    26 publications · 1.9K citations

    24

    h-index

  3. RM
    R. Maiolino

    University of Cambridge, United Kingdom

    30 publications · 4.2K citations

    23

    h-index

  4. JP
    Jean P. Brodie

    University of California, Santa Cruz, United States

    22 publications · 1.4K citations

    22

    h-index

  5. LJ
    Lisa J. Kewley

    Australian National University, Australia

    26 publications · 3.9K citations

    22

    h-index

1–5 of 4.2K

Venues

  1. The Astrophysical Journal

    ApJ · 517 publications · 52.7K citations

    116

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    498 publications · 42.4K citations

    112

    h-index

  3. Astronomy and Astrophysics

    226 publications · 19.3K citations

    75

    h-index

  4. The Astronomical Journal

    AJ · 113 publications · 9.8K citations

    55

    h-index

  5. The Astrophysical Journal Letters

    63 publications · 4.2K citations

    39

    h-index

1–5