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Challenges in Stellar Models from Helioseismology to Asteroseismology

Published online by Cambridge University Press:  30 March 2016

Sylvaine Turck-Chièze
SAp/DAPNIA/DSM/CEA CE Saclay, 91191 Gif sur Yvette, France
Phu Anh Phi Nghiem
SAp/DAPNIA/DSM/CEA CE Saclay, 91191 Gif sur Yvette, France
Laurent Piau
SAp/DAPNIA/DSM/CEA CE Saclay, 91191 Gif sur Yvette, France, ULB/IAA CP 226, Boulevard du Triomphe, B-1050 Bruxelles, Belgium


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Experience in helioseismology provides guidance for modeling challenges in asteroseismology. It guides choices of targets and conditions of observation. The main objectives are the interplay between rotation and convection and the knowledge of the internal magnetic field. Progress on the structure of the outer layers is crucial to avoid mode identification problems.

I. Joint Discussions
Copyright © Astronomical Society of Pacific 2005


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