Table 1.
Initial parameters of the star cluster models.
| fbin | 50% (P:rnd) | 50% (P:uni) | 100% |
|---|---|---|---|
| N | 2404 | 2404 | 2404 |
| Mcl [M⊙] | 1318.1 | 1318.1 | 1318.1 |
| rh [pc] | 0.258 | 0.263 | 0.262 |
| tcr [Myr] | 0.219 | 0.221 | 0.221 |
| trh [Myr] | 3.67 | 3.77 | 2.68 |
| seg | |||
| m5 [M⊙] | 100.5 | 116.8 | 113.7 |
 |
31.3 | 31.7 | 29.6 |
 |
9.7 | 9.7 | 9.6 |
| non | |||
| m5 [M⊙] | 2.61 | 3.84 | 2.74 |
 |
33.3 | 33.9 | 31.3 |
 |
10.3 | 10.1 | 9.7 |
| # runs | 85 | 50 | 80 |
| # runs (eig) | 160 | 80 | 90 |
Notes. The columns represent initial binary fractions and pairings. The top part shows: the number of stars, mass of the cluster, half-mass radius, crossing time, and median relaxation time of the models. The middle two parts show: the mass of the five innermost stars, the density enclosed in the central 0.1 pc and in the half-mass radius for both seg and non initial conditions. The mean values for each model are given. The bottom part shows the number of runs, which is the same for seg and non models, but differs for models with and without eigenevolution.
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