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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

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