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.
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CITATION STYLE
APA
De Cat, P., Daszyńska-Daszkiewicz, J., Briquet, M., Dupret, M.-A., Scuflaire, R., De Ridder, J., … Aerts, C. (2004). g -mode pulsations in slowly pulsating B stars. International Astronomical Union Colloquium, 193, 195–203. https://doi.org/10.1017/s0252921100010617
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