Table 1.
Simulations that do not include stellar mergers.
| Numbers | N | Mstars [M⊙] | Mext/Mstars | Rv [pc] | tcc/tcross |
|---|---|---|---|---|---|
| 1 | 1000 | 104 | 0.0 | 1.0 | 456 |
| 2 | 1000 | 104 | 0.1 | 1.0 | 460 |
| 3 | 1000 | 104 | 0.5 | 1.0 | 1 820 |
| 4 | 1000 | 104 | 1.0 | 1.0 | 6 553 |
| 5 | 10 000 | 104 | 0.0 | 1.0 | 2 306(a) |
| 6 | 10 000 | 104 | 0.1 | 1.0 | 3 377(a) |
| 7 | 10 000 | 104 | 0.5 | 1.0 | 13 519(a) |
| 8 | 10 000 | 104 | 1.0 | 1.0 | 51 889(a) |
Notes. Summary of simulations that do not include stellar mergers showing the number of particles, the cluster mass, the ratio of external potential to cluster mass, the virial radius and the ratio of core collapse time to crossing time in Cols. 1, 2, 3, 4, 5 and 6 respectively.
Crossing time calculated using Eq. (1) with q = Mext/Mstars = 1.0.
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