Subdwarf Stars

Subdwarf Stars is a stellar classification category denoting stars that lie below the main sequence in the Hertzsprung-Russell diagram and are distinguished by their lower luminosity and higher surface temperature compared to typical main-sequence stars of similar spectral type, often associated with evolved or metal-poor stellar populations.

609

Publications

33.3K

Citations

1.2K

Authors

464

Institutions

Publications per year

2017–2026

135

Variants

Subdwarf

Authors

1.2K

  1. UH
    U. Heber

    University of Würzburg, Germany

    75 publications · 4.1K citations

    35

    h-index

  2. SG
    S. Geier

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    51 publications · 2K citations

    29

    h-index

  3. RH
    R. H. Østensen

    KU Leuven, Belgium

    62 publications · 2.4K citations

    29

    h-index

  4. GF
    G. Fontaine

    Université de Montréal, Canada

    35 publications · 1.9K citations

    26

    h-index

  5. SC
    S. Charpinet

    Centre National de la Recherche Scientifique, France

    33 publications · 1.8K citations

    24

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 173 publications · 11.9K citations

    52

    h-index

  2. Astronomy and Astrophysics

    112 publications · 4.8K citations

    43

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    113 publications · 6.4K citations

    40

    h-index

  4. The Astronomical Journal

    AJ · 48 publications · 3.3K citations

    29

    h-index

  5. The Astrophysical Journal Supplement Series

    15 publications · 686 citations

    14

    h-index

1–5