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Some Masses For Population I and II Cepheids

Published online by Cambridge University Press:  12 April 2016

R. B. Kidman
Affiliation:
Theoretical Division, Los Alamos National Laboratory, University of California
A. N. Cox
Affiliation:
Theoretical Division, Los Alamos National Laboratory, University of California

Extract

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The masses of Cepheids can be obtained in several ways. If a Cepheid luminosity is known from membership in a galactic cluster, the mass-luminosity relation obtained from stellar evolution theory gives its mass. This evolution mass depends slightly on the composition, that is, the mass fraction of helium, Y, and on the the mass fraction of all the heavier elements, Z, but as we shall see later, the composition dependence is small.

Type
Part IV. Population II Cepheids
Copyright
Copyright © Cambridge University Press 1985

References

Becker, S. A., Iben, I., and Tuggle, R. S. (1977). Ap. J. 218, 633.CrossRefGoogle Scholar
Cox, A. N. (1979). Ap. J. 229, 212.CrossRefGoogle Scholar
Fernie, J. D. & McGonegal, R. (1983). Ap. J. 275, 732.CrossRefGoogle Scholar
Kraft, R. P. (1961). Ap. J. 134, 616.10.1086/147184CrossRefGoogle Scholar
Pel, J. W. (1978). Astr. Ap. Suppl. 31, 489.Google Scholar
Schmidt, E. G. (1984). Ap. J., in press.Google Scholar
Vandenberg, D. A. & Bridges, T. J. (1984). Ap. J. 278, 679.CrossRefGoogle Scholar
Zinn, R. & King, C. R. (1982). Ap. J. 262, 700.CrossRefGoogle Scholar