Open Access
Table A.1.
List of N-body simulations of the star cluster.
| Name | rvir/pc | ρc/(M⊙ pc−3) | IMF | m/M⊙ | ⟨m⟩/M⊙ |
|---|---|---|---|---|---|
| R07_NoImf | 0.7 | 3.5 ⋅ 104 | eq. mass | — | 0.38 |
| R07_Sal3 | 0.7 | 3.5 ⋅ 104 | Salpeter | [0.15, 3] | 0.38 |
| R07_Sal6 | 0.7 | 3.5 ⋅ 104 | Salpeter | [0.15, 6] | 0.42 |
| R07_Kr6 | 0.7 | 3.5 ⋅ 104 | Kroupa | [0.1, 6] | 0.48 |
| R13_NoImf | 1.3 | 5.5 ⋅ 103 | eq. mass | — | 0.38 |
| R13_Sal3 | 1.3 | 5.5 ⋅ 103 | Salpeter | [0.15, 3] | 0.38 |
| R13_Sal6 | 1.3 | 5.5 ⋅ 103 | Salpeter | [0.15, 6] | 0.42 |
| R13_Kr3 | 1.3 | 5.5 ⋅ 103 | Kroupa | [0.1, 3] | 0.43 |
| R13_Kr6 | 1.3 | 5.5 ⋅ 103 | Kroupa | [0.1, 6] | 0.48 |
| R30_NoImf | 3.0 | 5.0 ⋅ 102 | eq. mass | — | 0.38 |
| R30_Sal3 | 3.0 | 5.0 ⋅ 102 | Salpeter | [0.15, 3] | 0.38 |
| R30_Sal6 | 3.0 | 5.0 ⋅ 102 | Salpeter | [0.15, 6] | 0.42 |
Notes. For each simulation, the following initial parameters are given: the virial radius, the core density, the IMF and its mass range, and the mean stellar mass. The total mass of each model is 104 M⊙.
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