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The Chromospheric Spectrum and the Atmosphere of 31 Cygni
Published online by Cambridge University Press: 14 August 2015
Extract
The binary 31 Cygni is not, in the ordinary sense, an unstable star. Nevertheless, the organizers of this symposium have invited the present paper as a discussion of additional recent evidence of random motions of masses of gas in the atmospheres of the late-type giant components of certain double stars.
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- V. Phenomena of Instability in Binary Systems
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- Copyright © Cambridge University Press 1957