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The pulsation-rotation interaction: Greatest hits and the B-side

Published online by Cambridge University Press:  18 February 2014

Rich Townsend
Rich Townsend*
Affiliation:
Department of Astronomy, University of Wisconsin-Madison, Madison, WI 53706, USA email: townsend@astro.wisc.edu
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Abstract

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It has long been known that rotation can have an appreciable impact on stellar pulsation — by modifying the usual p and g modes found in the non-rotating case, and by introducing new classes of modes. However, it's only relatively recently that advances in numerical simulations and complementary theoretical treatments have enabled us to model these phenomena in any great detail. In this talk I'll review highlights in this area (the ‘Greatest Hits’), before considering the flip side (or the ‘B-side’, for those of us old enough to remember vinyl records) of the pulsation-rotation interaction: how pulsation can itself influence internal rotation profiles.

Keywords

stars: oscillationsstars: interiorsstars: rotationhydrodynamicswaves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 153 - 160
Copyright
Copyright © International Astronomical Union 2014 

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