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g-mode pulsations in slowly pulsating B stars
Published online by Cambridge University Press: 12 April 2016
Abstract
In this paper, we give an updated overview of the observed characteristics of g-mode pulsations in slowly pulsating B stars. These characteristics are based on the combined results of linear nonadiabatic analysis of the oscillations and a photometric and spectroscopic mode identification for a sample of 13 members. For 4 stars, at least one mode is stable in all the considered theoretical models.
- Type
- Part 4. Early-type stars: B, A and F pulsators
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 195 - 203
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
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