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- W2962959246 abstract "Abstract Until very recently the physical mechanism driving oscillations in β Cep and other early type stars has been a mystery. The breakthrough came with the publication of new OPAL and OP opacity data. Model calculations with the new opacities have demonstrated that the pulsations are driven by the familiar K -mechanism, acting in the metal opacity bump at T ≈ 2 × 10 5 K. The mechanism excites the low order p - and g -modes in the upper part of the instability strip and the high order g -modes in the lower part of the strip. The theoretical instability domains agree well with the observed domains of the β Cep and the SPB stars. In this review I present these recent theoretical results and discuss their consequences for our understanding of B stars pulsations." @default.
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- W2962959246 date "1995-01-01" @default.
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- W2962959246 title "New Results on Pulsating OB Stars" @default.
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- W2962959246 doi "https://doi.org/10.1017/s0252921100036769" @default.
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