Figure 5.
Histograms of the actual galaxy mass (top), total stellar mass in clusters (middle), and mass of the most massive star formed in clusters (bottom) for four different slug simulations with 5000 realizations each. The three simulations labelled as fc consist of the default slug CMF and different choices of the fraction of stars formed within clusters. The bottom panel compares instead two simulations with fc = 1, but for two different choices of CMF (slug's default and a CMF truncated at 100 M⊙).

Histograms of the actual galaxy mass (top), total stellar mass in clusters (middle), and mass of the most massive star formed in clusters (bottom) for four different slug simulations with 5000 realizations each. The three simulations labelled as fc consist of the default slug CMF and different choices of the fraction of stars formed within clusters. The bottom panel compares instead two simulations with fc = 1, but for two different choices of CMF (slug's default and a CMF truncated at 100 M).

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