Fig. 15.
Rmean and age relation for the sample of thin-disc stars investigated in this work (blue dots) and in Nissen et al. (2020) (magenta diamonds). This figure shows that in the Nissen et al. (2020) sample, young stars predominantly have larger Rmean. This causes a larger intercept in the [Y/Mg] and age relation in Nissen et al. (2020) than in this work.
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