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Radial Pulsations of δ Scuti Stars: Theory in Comparison with Observations

Published online by Cambridge University Press:  14 August 2015

A. A. Pamjatnykh
A. A. Pamjatnykh*
Affiliation:
Astronomical Council of the U.S.S.R. Academy of Sciences, Moscow

Abstract

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In this paper the pulsations of δ Sct star models are compared with observational data. The locations of the blue edges of the instability strips were computed as a function of helium abundance. Linear non-adiabatic pulsations were computed following Dziembowski's programme.

Type
Part 4 / δ Scuti Stars
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 247 - 250
Copyright
Copyright © Reidel 1975 

References

Baglin, A., Breger, M., Chevalier, C., Hauck, B., Le Contel, J. M., Sareyan, J. P., and Valtier, J. C.: 1973, Astron. Astrophys. 23, 221.Google Scholar
Breger, M.: 1974, Astrophys. J. 192, 75.Google Scholar
Christy, R. F.: 1966, Astrophys. J. 144, 108.Google Scholar
Cox, A. N., King, D. S., and Tabor, J. E.: 1973, Astrophys. J. 184, 201.Google Scholar
Crawford, D. L.: 1970, in Slettebak, A. (ed.), Stellar Rotation, p. 204.Google Scholar
Iben, I.: 1967, Ann. Rev. Astron. Astrophys. 5, 571.Google Scholar
Lindeman, E. and Hauck, B.: 1973, Astron. Astrophys. Suppl. 11, 119.Google Scholar
Vauclair, G., Vauclair, S., and Pamjatnykh, A. A.: 1974, Astron. Astrophys. 31, 63.Google Scholar
Pamjatnykh, A. A.: 1973, Nauchn. Informatsii 27, 99.Google Scholar