Fig. 6.
Ratio of heavy (Ba, La, Ce, Nd) and light (Sr, Y, Zr) s-process dominated element abundances with respect to [Fe I/H] compared with the GCE model predictions by Prantzos et al. (2018) (cyan line) and the thin-disc model by Pagel & Tautvaisiene (1997) (black line). Our results are marked as blue circles for the thin-disc and as red triangles for the thick-disc stars.
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