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Stellar ages from asteroseismology: a few examples

Published online by Cambridge University Press:  01 October 2008

Sylvie Vauclair
Sylvie Vauclair*
Affiliation:
Laboratoire d'Astronomie de Toulouse-Tarbes, Université de Toulouse, 14 Avenue Edouard Belin, 31400 Toulouse, France email: sylvie.vauclair@ast.obs-mip.fr
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Abstract

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Asteroseismology is a powerful tool to derive stellar ages, masses, gravities, radii, etc. Precise determinations of these parameters need deep analyses for each individual stars. Approximate theories are not efficient enough. Here I present results for two stars, μ Arae and ι Hor, which have both been observed during eight nights with the HARPS spectrograph in La Silla. I also show that important constraints can be obtained on core overshooting using the same techniques.

Keywords

stars: atmospheresinteriorsfundamental parametersoscillationstechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S258: The Ages of Stars , October 2008 , pp. 443 - 448
Copyright
Copyright © International Astronomical Union 2009

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