Table 1
Properties of the presented cluster models.
| ID | N stars |
|
SFE | N(M) | N sim |
| [pc] | |||||
|
|
|||||
| LK 1 | 30 000 | 1.3 | 0.2-1.0 | IMF | 15 |
| LK 1b | 30 000 | 1.3 | 0.2-1.0 | single | 15 |
| LK 2 | 30 000 | 4.6 | 0.2-0.3 | IMF | 15 |
| LK 3 | 45 000 | 1.3 | 0.3 | IMF | 15 |
| LK 4 | 15 000 | 1.3 | 0.3 | IMF | 31 |
| LK 5 | 30 000 | 3.0 | 0.3 | IMF | 15 |
| CK 1 | 30 000 | 0.1 | 0.3-0.7 | IMF | 7 |
| CK 2 | 30 000 | 0.2 | 0.6-0.7 | IMF | 5 |
Notes. ID stands for the identifier, the second column the number of stars, the third column the initial cluster radius (for a definition see main Sect. 2), the fourth column the range of investigated SFEs, N(M) the used mass representation, and the last column the number of simulations performed for the given set-up.
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