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Hydrodynamic Models of Population II Cepheids

Published online by Cambridge University Press:  12 April 2016

Yu.A. Fadeyev  and
A. B. Fokin
Yu.A. Fadeyev
Affiliation:
Astronomical Council of the Academy of Sciences of the USSR, 48 Pjatnitskaya St., Moscow 10917, USSR
A. B. Fokin
Affiliation:
Astronomical Council of the Academy of Sciences of the USSR, 48 Pjatnitskaya St., Moscow 10917, USSR

Extract

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This is a short report on hydrodynamic modelling for BL Her and W Vir pulsating variables. We present only a qualitative summary of the results obtained, whereas detailed paper will appear soon.

We studied radial self-exciting stellar oscillations with convection ignored. The Massevitch I mixture (X=0.7, Z=0.004) was assumed for calculating the opacity coefficient. All models have a mass M=0.6Mʘ, but their absolute magnitudes are in the range from -0.5 to -3 mag. The study covers the period range from 1.3 to 20 days.

Type
Part IV. Population II Cepheids
Information
International Astronomical Union Colloquium , Volume 82: Cepheids: Theory and Observations , 1985 , pp. 254 - 255
Copyright
Copyright © Cambridge University Press 1985

References

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Whitney, C. A. (1983). Stellar acoustic. I. Astrophys. J., 274, No.2, 830–839.CrossRefGoogle Scholar