Volume 441, Number 3, October III 2005
|Page(s)||1079 - 1086|
|Section||Stellar structure and evolution|
|Published online||23 September 2005|
Asteroseismic diagrams for solar-type stars
Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium e-mail: firstname.lastname@example.org
2 Observatoire de Paris, LESIA, CNRS UMR 8109, 92195 Meudon, France
Accepted: 18 June 2005
We explore the feasibility of applying the Christensen-Dalsgaard diagram to real asteroseismic data and provide quantitative measures of the uncertainty associated with the results. We also propose a new kind of seismic diagram, based on the determination of the locations of sharp acoustic features inside a star. We show that by combining the information about the position of the base of the convective envelope or the ionisation zone with a measure of the average large separation, it is possible to constrain the unknown chemical composition or the various parameters characterising the physical processes in the stellar interior. We demonstrate the application of this technique to the analysis of mock data for a CoRoT target star.
Key words: stars: oscillations / stars: interiors
© ESO, 2005
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