Fig. 11.
Abundance ratios [Ba/Y] vs. age in cluster and thin-disc stars (symbols as in Fig. 10) for the three radial ranges: 6.2 kpc < RGC < 8.2 kpc (left panels), RGC < 6.2 kpc (central panels) and RGC > 8.2 kpc (right panels). For each radial bin, we divide the plot into three metallicity ranges: below solar [Fe/H] < − 0.1 (panels in the upper row), solar −0.1 < [Fe/H] < +0.1 (panels in the central row) and super solar [Fe/H] > +0.1 (panels in the lower row).
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