Fig. 2.
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[Sr/Fe], [Zr/Fe], [Mo/Fe], and [Ru/Fe] with respect to [Fe/H] given for the giant stars in our sample (magenta points), the dwarf stars by Mishenina et al. (2019b), Mishenina et al. (2019a, 2013) (thin disk stars as black points, and thick disk stars as red points). The data from Forsberg et al. (2019) (Zr) and Forsberg et al. (2022) (Mo) are shown as blue points, while those from Tautvaišienė et al. (2021) – Sr and Zr I – are shown as open purple circles, and Zr II as open green triangles.
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