Fig. 11
Stars [Mg/Fe] as a function of [Fe/H] for the Fornax model, at t = 14 Gyr. On top, the RIMFS scheme is compared to the CIMFS, while on the bottom it is compared to the OIMFS scheme. From left to right, the panels show the effect of the increase in resolution. The yellow curve shown on the bottom of each plot corresponds to the observed dispersion in [Mg/Fe] extracted from all stars of Fig. 1.
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