Open issues in probing interiors of solar-like oscillating main sequence stars 1. From the Sun to nearly suns
arXiv:1102.0247 · doi:10.1088/1742-6596/271/1/012031
Abstract
We review some major, open issues in the current modelling of low and intermediate mass, main sequence stars based on seismological studies. In the present paper, the solar case is discussed together with current problems that are common to the Sun and stars with a structure similar to that of the Sun. Several additional issues specific to main sequence stars other than the Sun are reviewed and illustrated with a few stars observed with CoRoT in a companion paper.
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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