On the evolutionary state of beta cephei stars.
Low rotational velocities and period analyses of Beta Cephei variables lead to hypothesis that they are nonrotating stars undergoing radial oscillations
STELLAR EVOLUTION↗
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Low rotational velocities and period analyses of Beta Cephei variables lead to hypothesis that they are nonrotating stars undergoing radial oscillations
Stellar pulsational instability phenomena calculated numerically for infinitesimal amplitude of central core motion