Fig. A.1.
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Temporal evolution of the black hole cluster radius, R, from its representative initial value R0 = 0.1 pc. The cluster consists of N = 1000 equal mass black holes with mBH = 10 M⊙. The total mass of the gas, Mg, within the cluster is set to Mg = ηgMBH = ηgNmBH = 104 M⊙, i.e. ηg = 1. The cluster reaches the relativistic phase of its collapse at time trel ≈ 1.9 Myr.
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