Table 1
Initial conditions and characteristics of the explored MHD models.
| ID (M⊙) | μ | ℳ | Time | Mstar | rdisk |
|---|---|---|---|---|---|
| (Kyr) | (M⊙) | (au) | |||
| (1) | (2) | (3) | (4) | (5) | (6) |
| μ3ℳ0; (0.06) | 3.33 | 0 | 62.08 | 0.06 | 17.64 |
| μ3ℳ0; (0.18) | 3.33 | 0 | 67.80 | 0.18 | 20.71 |
| μ3ℳ0; (0.30) | 3.33 | 0 | 80.40 | 0.30 | 22.07 |
| μ10ℳ0; (0.07) | 10.00 | 0 | 53.52 | 0.07 | 38.38 |
| μ10ℳ0; (0.18) | 10.00 | 0 | 63.83 | 0.18 | 41.83 |
| μ10ℳ0; (0.30) | 10.00 | 0 | 81.43 | 0.30 | 41.81 |
| μ3ℳ1; (0.06) | 3.33 | 1 | 79.28 | 0.06 | 19.78 |
| μ3ℳ1; (0.18) | 3.33 | 1 | 92.41 | 0.18 | 17.80 |
| μ3ℳ1; (0.30) | 3.33 | 1 | 124.82 | 0.30 | 26.20 |
| μ10ℳ1; (0.07) | 10.00 | 1 | 67.65 | 0.06 | 41.95 |
| μ10ℳ1; (0.18) | 10.00 | 1 | 79.84 | 0.18 | 22.52 |
Notes. Initial parameters of the four RAMSES models analyzed in this work (Cols. 1–3), and properties of each of the three outputs selected for analysis (Cols. 4–6). ID is the identification tag of the model output, ℳ is the initial Mach number, time is the physical time elapsed since the sink creation, Mstar is the protostar mass, and rdisk is the disk radius. In addition, βrot, which is the thermal to gravitational energy ratio, is equal to 0.04, and θ, which is the initial angle between the rotation axis and the magnetic field direction (which corresponds to the z-axis), was set to 30°.
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