Subdwarf B Pulsations

Subdwarf B Pulsations is a type of non-radial stellar oscillation observed in subdwarf B stars, distinguished by short-period photometric variations caused by gravity-mode and p-mode pulsations driven by iron-group opacity peaks in their evolved, helium-burning cores.

178

Publications

7.7K

Citations

472

Authors

214

Institutions

Publications per year

2017–2026

30

Authors

472

  1. SC
    S. Charpinet

    Centre National de la Recherche Scientifique, France

    43 publications · 2.8K citations

    30

    h-index

  2. GF
    G. Fontaine

    Université de Montréal, Canada

    36 publications · 2.5K citations

    27

    h-index

  3. RH
    R. H. Østensen

    KU Leuven, Belgium

    48 publications · 1.7K citations

    26

    h-index

  4. PB
    P. Brassard

    Université de Montréal, Canada

    30 publications · 2.3K citations

    24

    h-index

  5. AS
    A. S. Baran

    Uniwersytet Komisji Edukacji Narodowej w Krakowie, Poland

    37 publications · 1.1K citations

    21

    h-index

1–5 of 472

Venues

  1. Astronomy and Astrophysics

    49 publications · 2.1K citations

    30

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    48 publications · 1.6K citations

    27

    h-index

  3. The Astrophysical Journal

    ApJ · 28 publications · 2K citations

    22

    h-index

  4. The Astrophysical Journal Letters

    7 publications · 351 citations

    7

    h-index

  5. The Astrophysical Journal Supplement Series

    5 publications · 295 citations

    5

    h-index

1–5