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Nonlinear pulsational behaviour of BW Vulpeculae
Published online by Cambridge University Press: 26 May 2016
Extract
BW Vulpeculae is a large amplitude β Cephei-type star, pulsating with a single period of 0.20104 day. Its nonlinear modeling was first attempted by Pesnell & Cox (1980). Because the true instability mechanism was not known then, the pulsation amplitude was imposed in that study in an arbitrary fashion.
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- 1. Pulsation and Rotation
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- Copyright © Kluwer 1994