Table 1
All the models with the corresponding parameters.
| Model | tSF 1 (Myr) | εSF |  |
MIMF 4 (M⊙) | ṁmax (M⊙ yr−1) | Rv 6 (pc) | Nstars 7 | M̄MMO 8 (M⊙) | N̄col 9 | M̄lost,coll 10 (M⊙) |
|---|---|---|---|---|---|---|---|---|---|---|
| E1 | 2.0 | 0.1 | 0.142 | 400 610.8 | 10−4 | 1.0 | 7100 | 440 ± 21 | 5±1 | 70 ± 5 |
| E2 | 2.0 | 0.2 | 0.142 | 800 929.6 | 10−4 | 1.0 | 31 500 | 756 ± 215 | 19±6 | 226 ± 103 |
| E3 | 2.0 | 0.3 | 0.142 | 1 203 113.3 | 10−4 | 1.0 | 47 500 | 2266 ± 1710 | 42 ± 12 | 876 ± 741 |
| E4 | 2.0 | 0.1 | 0.142 | 400 610.8 | 10−3 | 1.0 | 7100 | 14 434 ± 3098 | 30±7 | 5323 ± 1310 |
| E5 | 2.0 | 0.1 | 0.238 | 400 610.8 | 10−4 | 1.0 | 7100 | 332± 12 | 3±1 | 0.0 ± 0.0 |
| E6 | 0.5 | 0.1 | 0.142 | 400 610.8 | 10−4 | 1.0 | 7100 | 4704 ± 21 | 41 ± 3 | 1766 ± 25 |
Notes. (1)Total time during which SF occurs. (2)SF efficiency. (3)Density increase of the background potential due to gas accretion onto the cluster. (4) Total mass of the IMF. (5)Maximum accretion rate allowed for individual stars. (6)Radius of the cluster. (7) Number of stars in the IMF. (8)Average mass of the most massive object. (9)Average number of collisions. (10) Average amount of total mass lost by the MMO during stellar collisions. Three simulations were performed for each model.
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