Table 1
Stellar parameters of comparison stars in Fig. 9.
| Star | log (L/L⊙) | T eff | Ṁ | ν∞ | BC | Ref. |
| (kK) | (10-6 M⊙yr-1) | (km s-1) | (mag) | |||
|
|
||||||
| ζ1 Sco (B1 Ia+) | 5.93 | 17.2 | 1.55 | 390 | –1.6 | 1 |
| P Cygni (B1 Ia+/LBV) | 5.85 | 19.0 | 30.0 | 185 | –1.8 | 2 |
| Mean WN9h | 5.7 | 27.6 | 18.5 | 450 | –2.9 | 3 |
Notes. Tabulation of the bolometric luminosity (L), effective temperature (Teff), mass loss rate (Ṁ), terminal wind velocity (ν∞) and bolometric correction (BC) for the comparison spectra in Fig. 9. The value for the final entry is the mean of the modelling results for the four WN9h stars analysed by the latter authors. The broadly comparable luminosities reveal that the changes in spectral morphology are primarily the result of changes in temperature and wind parameters.
Reference.
Clark et al. (2012b);
Najarro (2001); and
Crowther & Smith (1997).
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