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Fig. 7.

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Evolution of the system when the BH is released from rest at a radius of r = 1.5kpc (from top left to bottom right). The black arrow indicates the velocity vector. Large density fluctuations soon develop in the inner ∼1kpc where the BH potential becomes dominant. After t ≈ 100 Myr of evolution, strong density fluctuations appear, including large-scale voids (deep blue). The BH used in the calculation had a mass M = 1.25 × 107 M.

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