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Instability in Stars of Early Spectral Type

  • Otto Struve (a1)

Extract

This paper consists of two parts which, at first sight, are quite detached from each other: the pulsating variables of spectral types B to F, and the close spectroscopic binaries of the types of β Lyrae, UX Monocerotis and U Cephei. I shall show that there exists a connexion between these groups which, though still rather nebulous (in both senses of this word), promises to yield interesting results.

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Instability in Stars of Early Spectral Type

  • Otto Struve (a1)

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