Table 2
TS, AP, and BS distances.
| Model | TS | AP | BS | Analytic |
|---|---|---|---|---|
| B* = 1 G | 2.2 | 3.7 | 11.4 | 3.3 |
| B* =10 G | 1.9 | 3.0 | 12.3 | 3.3 |
| B* =50 G | 2.2 | 3.7 | 15.5 | 3.3 |
| Ṁ* = 1.2 · 10−15 Ṁ⊙ υsw = 250 km/s | 10.4 | 23 | 45 | 16.2 |
| Ṁ* = 1.2 · 10−15Ṁ⊙ υsw = 1000 km/s | 20 | 46 | 96 | 32.3 |
| Ṁ* = 2.6 · 10−16Ṁ⊙ υsw = 430 km/s | 7.8 | 15 | 37 | 10.9 |
Notes. TS, AP, and BS distances for the model runs discussed in Sect. 6. Note that in the cases where only the magnetic field strength was changed (rows 1 to 3), the analytic solutions are always identical because the magnetic field is neglected in Eq. (3). Rows 4 to 6 show the results based on assuming a magnetic field strength of B* = 1G while changing the mass-loss rate (in rows 4 and 5 set to 1.2 · 10−15 M⊙/yr) and the stellar wind speed (υsw = 250 km/s, row 4 and υsw = 1000 km/s, row 5). Row 6 shows the results for 2 · 10−16 M⊙/yr and υsw = 250 km/s.
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