Table 1
Properties of the presented cluster models.
| ID | Nstars |
|
SFE | tdur | texp | N(M) | Nsim |
|
|
|||||||
| A 1 | 30 000 | 1.3 | 0.1–0.3 | 0 | 1 | IMF | 15 |
| A 2 | 15 000 | 1.3 | 0.3 | 0 | 1 | IMF | 30 |
| A 3 | 5000 | 1.3 | 0.3 | 0 | 1 | IMF | 90 |
| A 4 | 2000 | 1.3 | 0.3 | 0 | 1 | IMF | 100 |
| A 5 | 500 | 1.3 | 0.3 | 0 | 1, 3 | IMF | 100 |
| B | 500 | 1.3 | 0.3 | 2 | 1 | IMF | 400 |
Notes. ID stands for the identifier, the second column depicts the number of stars, the third column denotes the initial cluster half-mass radius in pc, the fourth column shows the range of investigated SFEs, tdur stands for the duration of the gas expulsion phase in Myr, texp the time at which gas expulsion starts, N(M) indicates the used mass representation and the last column the number of simulations performed for the given set-up.
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