Table 1
Initial conditions.
| Name | N (106) | Mtot (106 M⊙) | rh,1P/rh,2P | rtidal (pc) | βt=0 |
|---|---|---|---|---|---|
| N2M | 2.0 | 1.273 | 20 | 97 | iso |
| N1M | 1.0 | 0.637 | 20 | 77 | iso |
| N1M-ra | 1.0 | 0.639 | 20 | 77 | ani |
| N05M | 0.5 | 0.319 | 20 | 61 | iso |
| N05M-wf | 0.5 | 0.319 | 20 | 97 | iso |
| N2M-r10 | 2.0 | 1.275 | 10 | 97 | iso |
| N1M-r10 | 1.0 | 0.638 | 10 | 77 | iso |
Notes. N is the total number of stars; Mtot is the total mass of the cluster; rh,1P/rh,2P is the initial ratio of the 1P to 2P half-mass radius; rtidal is the cluster tidal radius; and βt=0 denotes initial velocity anisotropy (‘iso’ for isotropic or ‘ani’ for anisotropic). All simulations begin with a ratio rh/rtidal equal to approximately 0.14 and rh,2P/rtidal equal to about 0.01 (0.02 for the N2M-r10 and the N1M-r10 simulations).
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