Fig. 10.
Comparison of [C/N] and age between the theoretical models by Salaris et al. (2015) and the open clusters in GES and APOGEE surveys. The models are computed for different metallicities. Their colour codes are shown in the legend. The clusters are divided into three metallicity bins: [Fe/H] ≤ −0.10 (light blue circles), −0.1 ≤ [Fe/H] ≤ +0.1 (pink circles), and [Fe/H] ≥ +0.1 (grey circles).
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