Fig. 3.
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Time evolution of the mass fraction for the simulations with an initial temperature of 8000 K, 5000 K, 3000 K, 1000 K, and 500 K, corresponding to the gas mass (blue zone), protostars in the cluster (green zone) and the escaped protostellar mass (orange zone). The vertical dotted black lines indicate the times when the protostars accreted 25%, 50%, and 75% of the gas mass.
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