Fig. 5
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Final BH spin with respect to final BH mass for our typical cluster with M⋆ = 106 M⊙, rc,⋆ = 1 pc, and a star formation efficiency of ε = 0.35. (a) Scatter diagram for one indicative run. We have circled {high-spin, low-mass} and {low-spin, high-mass} outliers. (b) Percentiles, median, and fit relation, expressed by Eq. (31), for ten runs.
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