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Fig. 2


Comparison of the radii based on the PARSEC stellar evolutionary models for Praesepe with other stellar radii derived for Galactic field stars. The isochrones shown in Fig. 1 are used. The interferometric radii collected by Boyajian et al. (2013) are shown by blue dots, those derived from the extrasolar planetary systems in the Kepler field (Winn et al. 2017) by deep gray dots, and hot Jupiter hosts elsewhere (Maxted et al. 2015, extended/updated for this study) by yellow dots. The inset shows the same kind of plot, but using the large compilation of transiting planet hosts by Hartman et al. (2016).

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