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.
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2.9K
Citations
176
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94
Institutions
Publications per year
2017–2026
6
Variants
Beta Cephei PulsatorsBeta Cephei Stars
Parents
74
A plea for reexamining heavy element opacities in stars
N. R. Simon · The Astrophysical Journal · 1982 · 187 citations
Natural Sciences, Astronomy, Physics +13
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South African Nuclear Energy Corporation (South Africa), South Africa
5 publications · 135 citations
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4
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South African Radio Astronomy Observatory
Cape Town, South Africa
11 h-index
14 publications
333 citations
KU Leuven
Leuven, Belgium
9 h-index
9 publications
365 citations

University of Wrocław
Wroclaw, Poland
9 h-index
9 publications
260 citations
University of Vienna
Vienna, Austria
6 h-index
6 publications
202 citations

University of Toronto
Toronto, Canada
5 h-index
5 publications
375 citations

Radboud University Nijmegen
Nijmegen, The Netherlands
5 h-index
5 publications
193 citations
Nicolaus Copernicus Astronomical Center
Warsaw, Poland
5 h-index
5 publications
256 citations

Centre National de la Recherche Scientifique
Paris, France
4 h-index
4 publications
61 citations
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27 publications · 861 citations
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10 publications · 322 citations
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ApJ · 11 publications · 487 citations
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AJ · 6 publications · 392 citations
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3 publications · 370 citations
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