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Title:
Precise characterisation of exoplanet-host stars parameters
Authors:
Vauclair, Sylvie
Affiliation:
AA(Institut de Recherches en Astrophysique et Planetologie, 14 avenue Edouard Belin, 31400, Toulouse, France )
Publication:
The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution, Proceedings of the International Astronomical Union, IAU Symposium, Volume 276, p. 30-33
Publication Date:
11/2011
Origin:
CUP
Keywords:
stars: abundances, stars: oscillations, stars: interiors
Abstract Copyright:
(c) 2011: Copyright © International Astronomical Union 2011
DOI:
10.1017/S1743921311019892
Bibliographic Code:
2011IAUS..276...30V

Abstract

Studying the internal structure of exoplanet-host stars compared to that of similar stars without detected planets is particularly important for the understanding of planetary formation. In this framework, asteroseismic studies represent an excellent tool for a better characterization of stars and for a precise determination of the stellar parameters like mass, radius, gravity, effective temperature. The detection of stellar oscillations is obtained with the same instruments as used for the discovery of exoplanets, both from the ground and from space, although the time scales are very different. Here I discuss some details about the characterization of exoplanethost stars from seismology and the importance of the helium and heavy element abundances in this respect.

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