Fig. 7

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13 Gyr isochrones from the Dartmouth database (Dotter et al. 2008) with [α/Fe]=0.4 and with [Fe/H]=−1.50 (top panels) and [Fe/H]=−0.75 (bottom panels). Isochrones with pristine helium content (Y=0.246 and Y=0.254 for the top- and bottom-panels, respectively) are shown in aqua and light red, while those enriched in helium (Y=0.33) are displayed in blue and black. The light-red and black isochrones have chemical compositions with carbon and oxygen depletion of 0.5 and 0.9 dex, respectively, along with a nitrogen enhancement of 1.2 dex. In contrast, the aqua and blue isochrones represent stars with [O/Fe]=0.4 and solar abundances of carbon and nitrogen.
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