A New Asteroseismic Diagram For Solar-type Stars
Astrophysics
2010-12-09 v1
Abstract
We 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 second helium ionisation zone with a measure of the average large separation, it is possible to constrain the unknown 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.
Keywords
Cite
@article{arxiv.astro-ph/0510644,
title = {A New Asteroseismic Diagram For Solar-type Stars},
author = {Anwesh Mazumdar},
journal= {arXiv preprint arXiv:astro-ph/0510644},
year = {2010}
}
Comments
2 pages, to appear in the proceedings of the "Stellar Pulsation and Evolution" conference, Monte Porzio Catone, June 2005