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Fig. 7
SNe Ia rate as a function of time. We show the case of the vDC, SAL, CAN, and MKDP IMFs. Since only the MKDP IMF does not scale linearly with initial stellar mass, MUCD, we show also the lines for MUCD = 107 M⊙ and 108 M⊙; for the other IMFs we chose to plot only 109 M⊙. The text gives more details.
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