Figure 2

Mass Segregation of BHs in a Realistic GC—The cumulative fraction of all objects that are BHs as a function of radius, taken from a realistic GC model with \(N=10^{6}\) initial particles and realistic stellar evolution after 100 Myr of evolution Rodriguez et al. (2018). At the central region of the core (\(r < 0.01\) \(R_{v}\)) the evolution is almost entirely dominated by the BHs, with 75% of all objects in that region being BHs