Fig. 15

The SN Ia rate normalized to the galaxy stellar mass as a function of time as predicted by our best models (Minf = 109 M⊙). The solid red, dash-dotted black, long-dashed magenta and short-dashed blue lines are for models M9b1, M9b2, M9b3, and M9b4, respectively. As a comparison, the shaded area shows the observed range of normalized SN Ia rate in the Irr galaxies, per century and per 1010 M⊙ (Mannucci et al. 2005).
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