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Asteroseismology of red giants to constrain angular momentum transport

Published online by Cambridge University Press:  23 January 2015

P. Eggenberger
P. Eggenberger*
Affiliation:
Geneva Observatory, University of Geneva, Maillettes 51, 1290, Sauverny, Switzerland email: patrick.eggenberger@unige.ch
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Abstract

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Asteroseismic data obtained by the Kepler spacecraft have led to the recent detection and characterization of rotational frequency splittings of mixed modes in red-giant stars. This has opened the way to the determination of the core rotation rates for these stars, which is of prime importance to progress in our understanding of internal angular momentum transport. In this contribution, we discuss which constraints can be brought by these asteroseismic measurements on the modelling of angular momentum transport in stellar radiative zones.

Keywords

stars: evolutionstars: interiorsstars: oscillationsstars: rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 165 - 170
Copyright
Copyright © International Astronomical Union 2015 

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