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Radial Pulsations of δ Scuti Stars: Theory in Comparison with Observations
Published online by Cambridge University Press: 14 August 2015
Abstract
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