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Variations of the Period of AH Virginis

Published online by Cambridge University Press:  12 April 2016

Gustav A. Bakos

Extract

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AH Virginis was discovered by GUTHNICK and PRAGER (1929) and since that time the system was observed photographically, visually and, more recently, photoelectrically. The variable belongs to the class of eclipsing binaries of the W UMa type. It has a period of 0.41 days and spectrographic as well as photometric elements have been derived by CHANG (1948) and BINNENDIJK (1960), respectively. The most interesting result of discussions by KWEE (1958), BINNENDIJK (1960), HERCZEG (1962), and PURGATHOFER and PROCHAZKA (1967) is the fact that the residuals between the observed and the computed epochs of minima cannot be represented by a linear relation and show the tendency of producing sudden variations in the period of the system.

Type
IV. Duplicity and its Consequences among the Intrinsic Variable Stars
Information
International Astronomical Union Colloquium , Volume 15: New Directions and Frontiers in Variable Stars Research , 1971 , pp. 293 - 296
Copyright
Copyright © Cambridge University Press 1971

References

Binnendijk, L., 1960, Astron. J. 65, 358.Google Scholar
Chang, Y. C., 1948, Astrophys. J. 107, 96.CrossRefGoogle Scholar
Herczeg, T., 1962, Veröff. Univ. Sternw. Bonn, No. 63.Google Scholar
Kwee, K. K., 1958, B.A.N. 14, 131.Google Scholar
Prager, R., 1929, Kleine Veröff. Berlin Babelsberg No. 6, 36.Google Scholar
Purgathofer, A., and Prochazka, F., 1967, Mitteil. Univ.-Sternw. Wien 13, 151.Google Scholar
Sterne, Th. E., 1960, An Introduction to Celestial Mechanics. Interscience Publishers, Inc., New York.Google Scholar