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Fig. 9


Probability density functions derived from asteroseismology for the parameters loq q(H), log q(core), Xcore(C+O), Teff, and L/L. The red-hatched regions between the two vertical solid red lines shows the 1σ range containing 68.3% of the distribution. The blue vertical dashed line corresponds to the value of the optimal model. In the panel showing the distribution for Teff, the filled circle is the spectroscopic value with its 1σ (solid horizontal line) and 3σ (dotted horizontal line) uncertainties.

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