Fig. 2.
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Ratio of the radii from the Pietrzyński et al. (2019) SBCR and from asteroseismology as a function of different stellar parameters. Top: Radius ratio as a function of the stellar mass as estimated by scaling relations. Bottom: Same as in the top panel but as a function of the metallicity [Fe/H]. Colour codes and line styles are as in Fig. 1.
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