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Fig. 6
Predicted effects of the initial metallicity of the SNIa progenitor on the X/Fe abundance ratios. The comparison is made using the N100_Z0.01, N100_Z0.1, N100_Z0.5, and N100 3D delayed-detonation models from Seitenzahl et al. (2013b). For comparison, the ICM average abundance ratios (inferred from Paper I) are also plotted.
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