Table 1
Initial conditions for our simulations.
| Mtot [ M⊙ ] | Rcluster [ pc ] | N ∗ | Q vir |
|
|
|||
| 300 | [0.1, 0.25, 0.5] | [20, 70, 205, 610] | [0.1, 0.5, 1.0] |
| 1000 | [0.1, 0.25, 0.5] | [70, 230, 680, 2045] | [0.1, 0.5, 1.0] |
| 3000 | [0.1, 0.25, 0.5] | [205, 680, 2045, 6135] | [0.1, 0.5, 1.0] |
| Model | Mtot [ M⊙ ] | Rcluster [ pc ] | N ∗ | Q vir |
|
|
||||
| Low-mass (LM) | 300 | [0.1, 0.25, 0.5] | 610 | 0.5 |
| Intermediate mass (IM) | 1000 | 0.25 | [70, 230, 680, 2045] | 0.5 |
| High-mass (HM) | 3000 | [0.1, 0.25, 0.5] | 2045 | 0.5 |
| Trap30 | 1000 | 0.25 | 680 | 0.5 |
| Trap90 | 300 | 0.25 | 610 | 0.5 |
Notes. The initial conditions are defined by four parameters: the total mass of the cluster Mtot, the virial radius of the cluster, Rcluster, the number of stars, N∗, which determines the fraction of mass in stars, and the virial ratio, Qvir. We labelled several simulations for ease of reference.
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