Fig. 11
Behaviour of 0.5 ×( [Mg/Fe]+[Ca/Fe]) as a function of [Fe/H] for the whole sample (grey squares) in comparison with (upper panel) the Milky Way stars (red circles, Edvardsson et al. 1993; Burris et al. 2000; Fulbright 2000; Stephens & Boesgaard 2002; Gratton et al. 2003; Reddy et al. 2003, 2006; Barklem et al. 2005; Bensby et al. 2005), Fornax (blue dots, Letarte et al. 2010; Lemasle et al. 2014), and Carina stars (cyan triangles, Lemasle et al. 2012; Fabrizio et al. 2015), and with (lower panel) LMC stars (green dots, Lapenna et al. 2012; Van der Swaelmen et al. 2013).
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