Beta Cephei Variables

Beta Cephei Variables is a subclass of pulsating variable stars characterized by short-period oscillations driven by opacity-mediated heat engine mechanisms in massive B-type stars, distinguished from other pulsators by their spectral type, short pulsation periods (typically 0.1–0.3 days), and pulsation modes dominated by low-order pressure and mixed modes.

74

Publications

2.9K

Citations

176

Authors

94

Institutions

Publications per year

2017–2026

6

Variants

Beta Cephei PulsatorsBeta Cephei Stars

Authors

176

  1. LA
    L. A. Balona

    South African Radio Astronomy Observatory, South Africa

    11 publications · 298 citations

    10

    h-index

  2. CA
    C. Aerts

    KU Leuven, Belgium

    8 publications · 339 citations

    8

    h-index

  3. AP
    A. Pigulski

    University of Wrocław, Poland

    6 publications · 143 citations

    6

    h-index

  4. CA
    C. A. Engelbrecht

    South African Nuclear Energy Corporation (South Africa), South Africa

    5 publications · 135 citations

    5

    h-index

  5. GH
    G. Handler

    University of Vienna, Austria

    4 publications · 64 citations

    4

    h-index

1–5 of 176

Venues

  1. 17

    h-index

  2. Astronomy and Astrophysics

    10 publications · 322 citations

    10

    h-index

  3. The Astrophysical Journal

    ApJ · 11 publications · 487 citations

    10

    h-index

  4. The Astronomical Journal

    AJ · 6 publications · 392 citations

    6

    h-index

  5. The Astrophysical Journal Supplement Series

    3 publications · 370 citations

    3

    h-index

1–5