Table 1
Initial conditions for the different simulations.
| Run | Mass of | Number of | R init | T init | α | t ff | Time |
| number | cloud | groups | (AU) | (K) | (Myr) | (Myr) | |
|
|
|||||||
| 1 | 1 M⊙ | 1 | 104 | 10 | 1.02 | 0.177 | 0.193 |
| 2 | 20 | 0.193 | |||||
|
|
|||||||
| 3 | 0.1 M⊙ | 1 | 103 | 10 | 1.02 | 0.018 | 0.021 |
| 4 | 20 | 0.022 | |||||
|
|
|||||||
| 5 | 10 M⊙ | 1 | 105 | 10 | 1.02 | 1.775 | 1.916 |
| 6 | 20 | 1.919 | |||||
|
|
|||||||
| 7 | 1 M⊙ | 1 | 5 × 103 | 10 | 0.51 | 0.063 | 0.062 |
| 8 | 2 × 104 | 5 | 1.02 | 0.502 | 0.551 | ||
| 9 | 104 | 5 | 0.51 | 0.177 | 0.177 | ||
| 10 | 5 × 103 | 20 | 1.02 | 0.063 | 0.068 | ||
Notes. Columns 2, 4 and 5 indicate the initial mass, radius, and temperature of the parent cloud, respectively. Column 3 specifies the number of frequency groups used in each run and the Col. 6 lists the values for the thermal to gravitational potential energy ratio α. Column 7 lists the free-fall time of the initial could, while the last column reports the time at the end of the simulation, when ρc = 6 × 10-2 g cm-3.
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