Fig. 7.

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Formation time of individual clusters as a function of their mass for each simulation. The top row shows the time between when the first star was born t0 and when the last star formed t100%, while the bottom row shows the time between when 10 and 90% of the total cluster mass has assembled. The horizontal dashed line denotes the main sequence lifetime of a 30 M⊙ star, which is the earliest time a star can deposit energy and momentum in a SN in our simulations.
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