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Theory of Pulsational Instabilities of Hot Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
Basic physical mechanism of the pulsational instability in OB stars is shortly reviewed. Similarities and differences in the driving effect acting in these objects and in the classical pulsating variables are emphasized. Updated theoretical instability domains in the H-R diagram, in the log g – log Teff and in the Period – log Teff diagrams are presented and compared with the observational data on β Cephei, SPB and some other types of hot variables.
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- Section V Pulsation
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- Copyright © Springer-Verlag 1999