Enhanced mass loss of very massive stars: Impact on the evolution, binary processes, and remnant mass spectrum

Open Access

Fig. 10.

Black hole number counts for BHs formed from stellar mergers (left) and nonmerging BBHs (right) for the simulations with Ṁ_rdw (top), Ṁ_{Γ_e} (middle), and Ṁ_L/M (bottom). The dashed pink lines indicate BH masses from single stellar evolution.

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