Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-25T01:49:35.736Z Has data issue: false hasContentIssue false

The Rates of Change of the Periods of SX Phe

Published online by Cambridge University Press:  25 April 2016

K. Thompson
Affiliation:
Department of Physics, Monash University, Melbourne, Vic 3168
D. W. Coates
Affiliation:
Department of Physics, Monash University, Melbourne, Vic 3168

Abstract

We present changes in the periods of the double-mode beat cepheid star SX Phe from 1951 to 1987 deduced from observed times of maximum light.

Type
Galactic and Stellar
Copyright
Copyright © Astronomical Society of Australia 1991

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Coates, D. W., Dale, M., Halprin, L., Robinson, J. and Thompson, K., 1979, Mon. Not. R. Astr. Soc., 187, 83.Google Scholar
Coates, D. W., Halprin, L. and Thompson, K., 1982, Mon. Not. R. Astr. Soc., 199, 135.Google Scholar
Femley, J. A., Jameson, R. F., Sherrington, M. R. and Sicilien, I., 1987, Mon. Not. R. Astr. Soc., 225, 451.Google Scholar
Goranskij, V. P., Kukaikin, B. V. and Samus, N. N., 1973, Variable Stars in Globular Clusters and in Related Systems, (ed. Femie, J. D.), Reidel Publishing Company, p. 101.Google Scholar
Pena, J. H., Peniche, R., Gonzalez, S. F. and Hobart, M. A., 1987, Stellar Pulsation, Proc. John P. Cox Memorial Conference, Los Alamos, (eds. Cox, A. N., Sparks, W. M. and Starrfield, S. G.), Lecture Notes in Physics, 274, 126, Springer-Verlag, Berlin.Google Scholar
Percy, J. R., Matthews, J. M. and Wade, J. D., 1980, Astron. Astrophys., 82, 172.Google Scholar
Poretti, E., 1988, I. B. V. S., 3167.Google Scholar
Sweigart, A. V. and Renzini, A., 1979, Astron. Astrophys., 71, 66.Google Scholar