Fig. 9.
Abundance ratios [X/Fe] vs. Age for the thin-disc stars (binned results, bin 0.1 dex wide, cyan squares) and the open clusters located in the solar neighborhood (green circles). The magenta dashed lines are the weighted linear fits to the cumulative sample of solar neighbourhood clusters and thin-disc field stars (see Table 6 for the coefficients) for stellar ages <8 Gyr.
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