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Fig. 18


The relation between [Mg/Fe] and [Fe/H] for our sample of RGB stars observed in Fornax, for the Milky Way halo and disk population (original references in Venn et al. 2004), the Sculptor dSph (DART, Hill et al. in prep.), the Sgr dSph (Sbordone et al. 2007; Monaco et al. 2005; Bonifacio et al. 2004) and Carina (Koch et al. 2008).

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