Fig. 2.
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Rate and fraction of stars formed in clusters. Top: SFR (filled line) and CFR (dotted line) as a function of time for all simulations. Both these quantities are measured on the same timescale (25 Myr). Bottom: the CFE as a function of time for all simulations. Dashed horizontal lines indicate the fractions of cluster mass to total stellar mass formed after 300 Myr (outside gray shaded region).
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