Open issues in probing interiors of solar-like oscillating main sequence stars: 2. Diversity in the HR diagram
arXiv:1102.0252 · doi:10.1088/1742-6596/271/1/012032
Abstract
We review some major open issues in the current modelling of low and intermediate mass, main sequence stars based on seismological studies. The solar case was discussed in a companion paper, here several issues specific to other stars than the Sun are illustrated with a few stars observed with CoRoT and expectations from Kepler data.
GONG 2010 - SoHO 24, A new era of seismology of the Sun and solar-like stars, To be published in the Journal of Physics: Conference Series (JPCS)
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