Fig. 8
HR diagram (same as Fig. 4) but stars observed by Blum et al. (2003) and Maness et al. (2007) are also plotted with black and blue circles, respectively. Overplotted are theoretical isochrones for ages (from left to right) 50 Myr, 100 Myr, 500 Myr, 1 Gyr, 5 Gyr, and 10 Gyr with solar metallicity using the Padova code (Girardi et al. 2000; Marigo et al. 2008).
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