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Fig. 2.

image

[Y/H], [Y/Mg], and [Mg/H] vs. age: sample of Gaia-ESO IDR5 clusters in three radial bins (RGC <  6.5 kpc in blue, 6.5 kpc < RGC <  9 kpc in green, and RGC >  9 kpc in pink) compared with results of the GCE for the thin disc at three RGC = 6, 8, and 10 kpc with the MAGN yields (continuous curves) and with the FRUITY yields (dot-dashed lines). The ages and RGC of open clusters are from Cantat-Gaudin et al. (2020). The star marks the abundance ratio at the solar age and Galactocentric distance.

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