Fig. 13.
Disc dissection of the APOKASC sample of Silva Aguirre et al. (2018) in high-α (violet points) and low-α (green points) sequence stars based on the chemical evolution model M1. Left panel: abundance ratios [α/Fe] vs. [Fe/H] for the APOKASC sample. The age metallicity relation and the temporal evolution of the [α/Fe] are shown in the middle and right panels, respectively.
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