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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

Dadaev, A. N., Pulkovo Bull. 19, No. 5, 31 (1954).Google Scholar
Kopal, Z., Jodrell Bank Ann. 1, 37 (1954).Google Scholar
Kuiper, G. P., Ap.J. 93, 133 (1941).CrossRefGoogle Scholar
Martynov, D. J., Publ. Engelhardt Obs. No. 25 (1948).Google Scholar
Mergentaler, J., Contr. Wroclaw Astr. Obs. No. 4 (1950).Google Scholar
Sofronicky, A. V., Pulkovo Bull. 19, No. 4, 1 (1953).Google Scholar
Svetchnikov, A. V., Variable Stars, 10, 262 (1955).Google Scholar
Wood, F. B., Ap.J. 112, 196 (1950).CrossRefGoogle Scholar