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Fig. 10


[Mg/Fe] and [α/Fe] for the 51 clusters from this work in comparison with disc and halo field stars from Venn et al. (2004), bulge field stars from Gonzalez et al. (2011), and clusters from Pritzl et al. (2005). In the panels with [Ti/Fe], [Ca,Ti/Fe], and [Mg,Ca,Ti/Fe], our results are [α/Fe] (see text for details).

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