Fig. 7
Mn/Fe yields expected from SNIa as a function of the initial metallicity of SNIa progenitors. The red solid line interpolates the estimated Mn/Fe ratio for four SNIa initial metallicites by Seitenzahl et al. (2013b), and is compared to the Mn/Fe measurement (expected from SNIa contributions) in the ICM (Paper I and this work) is shown in grey. The dotted blue line shows the solar metallicity (Lodders et al. 2009).
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