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The Effect of Binary Motion on Period Changes in RRLyrae Stars

Published online by Cambridge University Press:  12 April 2016

Extract

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The present investigation is to determine what apparent period changes if any, would result from binary motions. In particular it is important to know whether or not such apparent period changes could be mistaken for intrinsic period changes caused by evolution.

Type
IV. Duplicity and its Consequences among the Intrinsic Variable Stars
Copyright
Copyright © Cambridge University Press 1971

References

Allen, C. W., 1963, Astrophysical Quantities.Google Scholar
Coutts, C. M., and Sawyer-Hogg, H., 1969, David Dunlap Pub., 3, No. 1.Google Scholar
Epps, E., 1971, Observatory 91, 124.Google Scholar
Geyer, E. H., 1967, Z. f. A., 66, 16.Google Scholar
Jones, D. H. P., 1970, Proc. A.S.A., 1, 329.Google Scholar
Margoni, R., 1967, Asiago Cont. No. 198.Google Scholar
Sawyer, H. B., 1955, David Dunlap Pub., 2, No. 2.Google Scholar
Schlesinger, F., and Udick, S., 1912, Allegheny Pub., 2, 155.Google Scholar
Sistero, R. F., 1968, Inf. Bull, on Variable Stars No. 316.Google Scholar
Szeidl, B., 1965, Budapest Mitt. No. 58.Google Scholar
Wisniewski, W., 1971, Bamberg Colloquium.Google Scholar