Fig. 14
Color–magnitude diagram for the Hα emission-line stars (triangles). An extinction-correction was applied to obtain V0 and (V − I)0 values. The solid lines are evolutionary tracks from D’Antona & Mazzitelli (1997), for masses from 0.2 to 2.0 M⊙ and the dashed lines are their 0.1, 1, 5, 10 and 100 Myr isochrones. The stars are labeled as in Fig. 13.
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