Fig. A.1
Predicted X/Fe abundances from the Classical W7 model (SNIa), adopted from Iwamoto et al. (1999, brown) and Maeda et al. (2010, orange). The two models assume different electron capture rates, leading to different X/Fe ratios, both for intermediate-mass and Fe-group elements (see text). For comparison, the ICM average abundance ratios (inferred from Paper I) are also plotted.
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