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Phenomena of Non-Stability in Close Binary Systems

Published online by Cambridge University Press:  14 August 2015

D. J. Martynov
D. J. Martynov*
Affiliation:
Engelhardt Observatory, Kasan, U.S.S.R.

Extract

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(I) The non-stability of the components in close binary systems has been established in a number of systems, mainly among the eclipsing variables. It cannot be regarded as an unusual phenomenon.

Type
V. Phenomena of Instability in Binary Systems
Information
Symposium - International Astronomical Union , Volume 3: Non-Stable Stars , 1957 , pp. 138 - 143
Copyright
Copyright © Cambridge University Press 1957 

References

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