Fig. H.1.
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HR diagram for low-mass stars of Tr 14. Empty circles show data points. Open squares are median values of the bolometric luminosity for each spectral subclass, with error bars indicating 1-σ percentiles. Theoretical tracks from Baraffe et al. (2015) are shown as solid grey lines, whereas tracks from Siess et al. (2000) are plotted as dashed lines. Dotted lines show tracks for various masses of stars.
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