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Full Amplitude Models of 15 Day Cepheids

Published online by Cambridge University Press:  12 April 2016

B.C. Cogan ,
A.N. Cox  and
D.S. King
B.C. Cogan
Affiliation:
Los Alamos Scientific Laboratory
A.N. Cox
Affiliation:
Los Alamos Scientific Laboratory
D.S. King
Affiliation:
University of New Mexico

Abstract

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Numerical models of Cepheids have been computed with a range of effective temperatures and compositions. The amplitudes increase if the helium abundance increases or if the effective temperature decreases. The latter effect is contrary to observational data. The models also exhibit velocity amplitudes which are much lower than those observed.

Type
V. Cepheids of Populations I and II
Information
International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 419 - 424
Copyright
Copyright © Reidel 1980

References

Cogan, B.C., 1980, Astrophys. J., 239.Google Scholar
Cox, A.N., Hodson, S.W., and Davey, W.R., 1976, Proceedings of the Solar and Stellar Pulsation Conference, Cox, A.N. and Deupree, R.G., eds. (Los Alamos report LA-6544-C), pp. 188–201.Google Scholar
Deupree, R.G., and Varner, T.M., 1980, Astrophys. J., 237, pp. 558–562.CrossRefGoogle Scholar
Flower, P.J., 1977, Astron. Astrophys., 54, pp. 31–39.Google Scholar
Stellingwerf, R.F., 1975, Astrophys. J., 195, pp. 441–466.CrossRefGoogle Scholar
Stobie, R.S., 1968, Monthly Notices Roy. Astron. Soc., 144, pp. 485–510.CrossRefGoogle Scholar