Fig. 5
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Black hole mass distribution from binaries with MZAMS,1 > 50M⊙, for models adopting the S23 (solid blue line, solid fill) and C15 (dashed red line, hatched area) wind prescriptions. The shaded (hatched) areas indicate the BHs in BBHs, while the empty histograms display the single BHs from disrupted binaries, including BHs that form from stellar collisions.
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