Fig. 13
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Evolution of star formation for the clumps of 1000 and 500 M⊙ for seeds 1 and 2 (with the fiducial set of parameters, except for the mass). From left to right, we display the star formation rate, the maximum sink mass, the median sink mass as a function of the SFE, and the IMF at SFE=0.1. For the IMF, we combined seed 1 and 2 to enhance the statistics of the 500 M⊙ case.
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