Table 1
Parameters of the protostellar models.
| ID | μ | βrot | θ | M | tform [yr] |  [yr] |
 [yr] |
 [yr] |
|---|---|---|---|---|---|---|---|---|
| R1 | 3.33 | 0.01 | 30° | 0 | 55 428 | 2493 | 5991 | 13 484 |
| R2 | 3.33 | 0.04 | 30° | 0 | 60 328 | 2472 | 8760 | 19 509 |
| R3 | 10.0 | 0.04 | 30° | 0 | 50 987 | 5179 | 14 816 | 30 282 |
| R4 | 6.67 | 0.04 | 30° | 0 | 51 206 | 3693 | 8927 | 17 943 |
| R6 | 3.33 | 0.01 | 30° | 1 | 66 942 | 3618 | 12 321 | 30 486 |
| R7 | 3.33 | 0.04 | 90° | 0 | 56 006 | 2461 | 6001 | 13 532 |
| R8 | 6.67 | 0.01 | 30° | 1 | 57 132 | 2460 | 7331 | 16 413 |
| R9 | 10.0 | 0.04 | 90° | 0 | 49 636 | 5112 | 15 843 | 42 005 |
| R10 | 3.33 | 0.0025 | 30° | 0 | 52 577 | 2828 | 7015 | 12 982 |
Notes. Selected numerical models from Hennebelle et al. (2020). μ is the mass-to-flux ratio normalized by the critical value, βrot is the ratio between rotational energy and gravitational energy, 8 is the inclination angle of the initial rotation axis with respect to the magnetic field axis, and M is the initial Mach number. tform is the time at which the sink forms in the simulation, while 
and 
are the ages of the sink at which it reaches 0.1, 0.2, and 0.3 M⊙, respectively.
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