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Table 5.
Stellar and wind parameters of HD 191612 (left panel).
| Teff (kK) | 35 | ||
| log g | 3.5 | ||
| R* (R⊙) | 14.5 | ||
| v∞ (km s–1) | 2700 |  (km s–1) |
3963 |
| MṀ (M⊙ yr–1) | 1.6 × 10–6 | MṀB = 0 (M⊙ yr–1) | 1.1 × 10–6 |
| ⇒ RA(R*) | 2.7 |
Notes. Teff, log g, R∗, Ṁ, v∞ have been derived by Howarth et al. (2007), and Bp is adopted from Wade et al. (2011). For the ADM model, we adapted the mass-loss rate and terminal velocity at the pole (right panel), to be consistent with the MHD simulations from Fig. 9.
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