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23. Evidence for and against the binary nature of some Tio-he II-nebular variables, and the possible amplification of B-star eruptions by a cool companion

Published online by Cambridge University Press:  02 August 2017

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1. This problem might be deprecated as requiring for its solution more evidence than now exists; but, even though it cannot yet be conclusively solved, it will introduce some consideration of possible interactions between binary components and between different atmospheric regions of a single star, which may help to explain other peculiar variable spectra.

Type
Part IV Symposia
Copyright
Copyright © Cambridge University Press 1954

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