Fig. 11.
Comparison between age and [C/N] of the thin-disc RC giant modelled by Lagarde et al. (2017) (continuous lines in light blue, pink, and grey) and the clusters in GES and APOGEE. The clusters and models 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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