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Fig. 10

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[Mn/Fe] vs. [Fe/H]: present results, with the same symbols as in Fig. 7, compared with a) Ishigaki et al. (2013): thick disc and halo (blue squares); b) Sobeck et al. (2006): globular clusters (blue crosses); field stars (red squares), bulge metal-rich globular clusters plus the old open cluster Cr261 with stellar parameters from the literature (green stars); c) Gratton (1989) (blue squares), and Prochaska et al. (2000) (thick disc: full magenta triangles).

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