Fig. 3.
Hertzsprung-Russel diagram with Siess et al. (2000) evolutionary tracks from 0.2 to 1.8 M⊙ (dashed lines). Isochrones corresponding to 1, 2, 3, 4, 5, and 10 Myr (solid lines) are also represented. The circles correspond to the values determined in this work and the squares to the values of Hillenbrand (1997), rescaled to the distances derived from the Gaia DR2 parallaxes.
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