Table 3.
Specific parameters used and obtained for the rotating wind models.
| vrot [km s−1] | 0 | 210 | 294 | 432 |
|---|---|---|---|---|
| Ω | 0 | 0.5 | 0.7 | 0.9 |
| Req [Rp] | 1 | 1.04 | 1.09 | 1.22 |
| Teff, p [kK] | 41.84 | 42.44 | 43.07 | 44.66 |
| Teff, eq [kK] | 41.84 | 40.61 | 39.28 | 35.20 |
| Ṁ [10−6 M⊙ yr−1] | 2.70 | 2.73 | 2.79 | 2.93 |
| v∞, p [km s−1] | 2781 | 2989 | 3255 | 3159 |
| v∞, eq [km s−1] | 2781 | 2651 | 2556 | 2273 |
Notes. For a given stellar luminosity L* = 106 L⊙, stellar mass M* = 52.5 M⊙, and polar radius Rp = 19 R⊙, rows two to eight display the rotation parameter Ω, the equatorial radius Req, the polar and equatorial effective temperature Teff, p, Teff, eq, the total mass loss rate Ṁ, and the polar and equatorial terminal velocity v∞,p, v∞,eq, for different equatorial rotation speeds vrot.
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