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Table 3
Stellar and wind parameters of our model grid used to compare synthetic N ii/N iii profiles from fastwind and cmfgen.
| Luminosity class V | ||||||
| Model | Teff | R∗ | log g | Ṁ | v∞ | β |
| (K) | (R⊙) | (cgs) | (10-6 M⊙ yr-1) | (km s-1) | ||
|
|
||||||
| d2v | 46 100 | 11.4 | 4.01 | 2.52 | 3140 | 0.8 |
| d4v | 41 010 | 10.0 | 4.01 | 0.847 | 2850 | 0.8 |
| d6v | 35 900 | 8.8 | 3.95 | 0.210 | 2570 | 0.8 |
| d8v | 32 000 | 8.0 | 3.90 | 0.056 | 2400 | 0.8 |
| d10v | 28 000 | 7.4 | 3.87 | 0.0122 | 2210 | 0.8 |
|
|
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| Luminosity class I | ||||||
| Model | Teff | R∗ | log g | Ṁ | v∞ | β |
| (K) | (R⊙) | (cgs) | (10-6 M⊙ yr-1) | (km s-1) | ||
|
|
||||||
| s2a | 44 700 | 19.6 | 3.79 | 12.0 | 2620 | 1.0 |
| s4a | 38 700 | 21.8 | 3.57 | 7.35 | 2190 | 1.0 |
| s6a | 32 740 | 24.6 | 3.33 | 3.10 | 1810 | 1.0 |
| s8a | 29 760 | 26.2 | 3.21 | 1.53 | 1690 | 1.0 |
| s10a | 23 780 | 30.5 | 2.98 | 3.90 | 740 | 1.0 |
Notes. The grid is a subset of the grid presented by Lenorzer et al. (2004).
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