Stellar type population changes in the cluster (a), near-tail (b), and the far-tail (c) for the M20000 model. Population evolution is shown for all stars, the main sequence (MS), white dwarfs (WDs), neutron stars (NSs) + black holes (BHs), subgiant (SGBs), red giant (RGBs), and the post-RGB population. The v_relax is shown for reference. Similar plots for M4641 and M1000 are shown in Figure A.7.