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Fig. 2.

image

Maximum BH mass achieved after gas accretion of an initial population of N = 500 BHs, with initial mass cutoff at 50 M, with respect to the half-mass radius rhm of the stellar cluster for ten samples of the BH population at each rhm. The vertical lines represent the range of maximum mass values achieved in all samples for a certain rhm. The gas is assumed to be exponentially depleted by 99% within tf = 10 Myr.

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