Table 2.
Parameters used to confront the stellar initial mass function inferred from the simulations with the analytical model stated in Sect. B.
| Name | Rc (pc) | cs (km s−1) | Va (km s−1) | V0 (km s−1) | Mtot, * (M⊙) | Mmax (M⊙) | Mmin (M⊙) |
|---|---|---|---|---|---|---|---|
| NMHD10f05 | 0.3 | 0.35 | 1 | 3 | 100 | 3 | 0.1 |
| IMHD10f05 | 0.3 | 0.35 | 1 | 3 | 150 | 8 | 0.1 |
| IMHD10f01 | 0.3 | 0.25 | 1 | 3 | 150 | 7 | 0.1 |
| IMHD100f05 | 0.3 | 0.35 | 0.3 | 3 | 150 | 7 | 0.1 |
| HYDROf05 | 0.3 | 0.35 | 0 | 3 | 150 | 7 | 0.1 |
| HYDROf01 | 0.3 | 0.25 | 0 | 3 | 150 | 3 | 0.1 |
Notes. Rc is the clump radius, cs is the typical sound speed, Va, the Alfvén speed, V0, the velocity dispersion, Mtot, * is the total accreted mass, Mmax, the mass of the most massive stars formed and Mmin is the smallest mass for which the comparison is meaningful.
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