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2005MNRAS.360..465T - Mon. Not. R. Astron. Soc., 360, 465-476 (2005/June-3)
Influence of the Coriolis force on the instability of slowly pulsating B stars.
TOWNSEND R.H.D.
Abstract (from CDS):
The implications of these results are discussed in the context of the observational scarcity of pulsation in B-type stars having significant rotation; various scenarios are explored to explain the apparent dichotomy between theory and observations. Furthermore, the possible significance of the findings to Be stars is briefly examined.
Abstract Copyright: 2005 RAS
Journal keyword(s): methods: numerical - stars: early-type - stars: emission-line, Be - stars: oscillations - stars: rotation - stars: variables: other
Simbad objects: 6
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