Table 1.
Initial conditions of simulations.
| fbinary (%) | rt/rM | N | Mtot [M⊙] | rt [pc] | trh [Gyr] | |
|---|---|---|---|---|---|---|
| Sim 1 (10 low 75) | 10 | 75 | 5 × 105 | 3.62 × 105 | 150 | 0.53 |
| Sim 2 (50 low 75) | 50 | 75 | 5 × 105 | 5.07 × 105 | 150 | 0.44 |
| Sim 3 (10 low 37) | 10 | 37 | 5 × 105 | 3.62 × 105 | 150 | 1.51 |
| Sim 4 (50 low 37) | 50 | 37 | 5 × 105 | 5.07 × 105 | 150 | 1.28 |
| Sim 5 (10 low 180) | 10 | 180 | 5 × 105 | 3.62 × 105 | 150 | 0.14 |
| Sim 6 (50 low 180) | 50 | 180 | 5 × 105 | 5.07 × 105 | 150 | 0.12 |
| Sim 7 (10 low 75−2M) | 10 | 75 | 20 × 105 | 7.26 × 105 | 150 |
Notes. In the first column, the original label of the simulations from Downing et al. (2010) is given in parentheses. The other columns list the binary fraction fbinary, the ratio of the truncation to the half-mass radius rt/rM, the total number of particles N (defined as the number of single stars plus the number of binary systems), the total mass Mtot, the truncation radius rt, and the half-mass relaxation time defined as in Downing et al. (2010).
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