Interstellar Abundances

Interstellar Abundances is a scientific construct that denotes the relative quantities of chemical elements and isotopes present in the diffuse interstellar medium, typically measured with respect to hydrogen and derived from spectroscopic observations of interstellar absorption lines.

810

Publications

62.1K

Citations

1.8K

Authors

625

Institutions

Publications per year

2017–2026

79

Variants

Interstellar Chemical Abundances

Authors

1.8K

  1. EH
    Eric Herbst

    The Ohio State University, United States

    23 publications · 2.2K citations

    21

    h-index

  2. DG
    Donald G. York

    University of Chicago, United States

    18 publications · 1.1K citations

    18

    h-index

  3. EB
    E. B. Jenkins

    Princeton University, United States

    16 publications · 1.4K citations

    16

    h-index

  4. AV
    A. Vidal‐Madjar

    Institut d'Astrophysique de Paris, France

    13 publications · 756 citations

    13

    h-index

  5. BD
    Blair D. Savage

    University of Wisconsin–Madison, United States

    13 publications · 2.4K citations

    13

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 375 publications · 30.8K citations

    84

    h-index

  2. Astronomy and Astrophysics

    75 publications · 6.9K citations

    43

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    86 publications · 4.2K citations

    36

    h-index

  4. The Astrophysical Journal Supplement Series

    23 publications · 2.2K citations

    20

    h-index

  5. The Astronomical Journal

    AJ · 15 publications · 527 citations

    13

    h-index

1–5