Stellar Pulsation Modes

Stellar Pulsation Modes is a theoretical construct in astrophysics that categorizes the distinct periodic oscillations in a star's brightness and radial velocity arising from intrinsic hydrodynamic instabilities, differentiated by their characteristic frequencies, spherical harmonic degrees, and underlying restoring forces such as pressure or gravity waves.

1.1K

Publications

55.7K

Citations

2.1K

Authors

634

Institutions

Publications per year

2017–2026

170

Authors

2.1K

  1. DW
    D. W. Kurtz

    University of Lancashire, United Kingdom

    70 publications · 3.5K citations

    38

    h-index

  2. GH
    G. Handler

    University of Vienna, Austria

    53 publications · 2.4K citations

    30

    h-index

  3. SC
    S. Charpinet

    Centre National de la Recherche Scientifique, France

    36 publications · 2.4K citations

    29

    h-index

  4. CA
    C. Aerts

    KU Leuven, Belgium

    52 publications · 2.7K citations

    29

    h-index

  5. HS
    Hideyuki Saio

    Tohoku University, Japan

    38 publications · 1.9K citations

    27

    h-index

1–5 of 2.1K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    346 publications · 17.5K citations

    69

    h-index

  2. The Astrophysical Journal

    ApJ · 220 publications · 12.8K citations

    57

    h-index

  3. Astronomy and Astrophysics

    216 publications · 10.2K citations

    54

    h-index

  4. The Astronomical Journal

    AJ · 29 publications · 1.3K citations

    18

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 17 publications · 687 citations

    16

    h-index

1–5