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Table 2.
Estimations of the Spitzer and turbulent resistivity parameters for the fully convective protostellar models adopted by Moss (2003).
| R* | T* | vc | ηS | ηturb |
|---|---|---|---|---|
| (R⊙) | (K) | (m s−1) | (cm2 s−1) | (cm2 s−1) |
| M* = 1 M⊙ | ||||
| 13 | 1.1 × 106 | 37.94 | 3.1 × 103 | 1.8 × 1014 |
| 6 | 2.3 × 106 | 33.35 | 9.6 × 102 | 7.4 × 1013 |
| 3 | 4.6 × 106 | 29.71 | 3.4 × 102 | 3.3 × 1013 |
| 2 | 6.9 × 106 | 27.77 | 1.9 × 102 | 2.1 × 1013 |
| 1.8 | 7.7 × 106 | 27.29 | 1.6 × 102 | 1.8 × 1013 |
| M* = 3 M⊙ | ||||
| 22 | 1.9 × 106 | 215.22 | 1.3 × 103 | 1.7 × 1015 |
| 15 | 2.8 × 106 | 201.91 | 7.3 × 102 | 1.1 × 1015 |
| 13 | 3.2 × 106 | 197.15 | 5.9 × 102 | 9.5 × 1014 |
| 11 | 3.8 × 106 | 191.74 | 4.6 × 102 | 7.8 × 1014 |
| 9 | 4.6 × 106 | 185.43 | 3.4 × 102 | 6.2 × 1014 |
| M* = 5 M⊙ | ||||
| 45 | 1.5 × 106 | 521.73 | 1.8 × 103 | 8.7 × 1015 |
| 30.5 | 2.3 × 106 | 488.98 | 9.9 × 102 | 5.5 × 1015 |
| 21.6 | 3.2 × 106 | 461.66 | 5.9 × 102 | 3.7 × 1015 |
| 19.3 | 3.6 × 106 | 453.07 | 5.0 × 102 | 3.2 × 1015 |
| 18 | 3.8 × 106 | 447.84 | 4.5 × 102 | 3.0 × 1015 |
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