Nebular Metallicity

Nebular Metallicity is the measure of the abundance of chemical elements heavier than helium in ionized gas regions of interstellar space, relative to hydrogen, used as an indicator of galactic chemical evolution and star formation history.

339

Publications

24.9K

Citations

1.3K

Authors

464

Institutions

Publications per year

2017–2026

79

Authors

1.3K

  1. DS
    D. Schaerer

    University of Geneva, Switzerland

    10 publications · 587 citations

    10

    h-index

  2. SC
    S. Charlot

    Institut d'Astrophysique de Paris, France

    10 publications · 1.4K citations

    10

    h-index

  3. GS
    G. Stasińska

    Centre National de la Recherche Scientifique, France

    8 publications · 981 citations

    8

    h-index

  4. RM
    R. Maiolino

    University of Cambridge, United Kingdom

    7 publications · 458 citations

    7

    h-index

  5. YI
    Y. I. Izotov

    Main Astronomical Observatory, Ukraine

    7 publications · 485 citations

    7

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 96 publications · 9.5K citations

    54

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    85 publications · 6.9K citations

    45

    h-index

  3. Astronomy and Astrophysics

    38 publications · 2.4K citations

    28

    h-index

  4. The Astronomical Journal

    AJ · 15 publications · 882 citations

    14

    h-index

  5. The Astrophysical Journal Letters

    9 publications · 362 citations

    9

    h-index

1–5