Fig. 9.
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HR diagram for low-mass stars of Tr 14. Filled circles show data points. Empty squares are the median values of the bolometric luminosity for each spectral subclass, with error bars indicating 1-σ percentiles. Theoretical tracks from Bressan et al. (2012) are shown as solid black lines. Dotted grey lines show tracks for 0.3, 0.7, 1, and 3 M⊙ stars.
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