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Fig. 8

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Probability density function for the stellar radius from asteroseismology. The filled circle with the solid horizontal line indicates the 1σ error associated to the relevant orbital solution from Vučković et al. (2007). The red-hatched region between the two vertical solid red lines is the 1σ range containing 68.3% of the radius distribution. The blue vertical dashed line corresponds to the radius of the optimal model solution of the lowest S2-value.

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