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Fig. 2
Number of SNII explosions, upper panel a); cumulative number of SNII, lower panel b), both as a function of time for a 2048 M⊙ stellar particle. The red lines correspond to the analytical IMF, (CIMFS), while the black lines correspond either to the RIMFS a) or the OIMFS b).
This figure is made of several images, please see below:
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