Table 1
Summary of simulation runs in this paper.
| ID | Stars | W 0 | Mass ratios | N ratios |
|
|
||||
| 32k3cW02 | 32 × 103 | 2 | 1:2:3 | 99:0.5:0.5 |
| 16k3cW02 | 16 × 103 | 2 | 1:2:3 | 98:1:1 |
| 16k4cW02 | 16 × 103 | 2 | 1:2:3:4 | 97.5:1:1:0.5 |
| 16k4cW02 | 16 × 103 | 2 | 1:2:3:4 | 97.75:1:1:0.25 |
| 16k3cW04 | 16 × 103 | 4 | 1:2:3 | 98:1:1 |
| 16k4cW04 | 16 × 103 | 4 | 1:2:3:4 | 97:1:1:1 |
Notes.The simulations either have three or four classes of mass. The number ratios and the mass ratios are given in the relevant columns in the table. The initial conditions are a King-model with dimensionless potential W0 as listed in the table. Primordial binary fraction is consistently 0 over the whole set of simulations.
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