Table 3
WLR parameters for Galactic early-type stars.
| Reference |
|
log D0 |
|
|
||
| Kudritzki & Puls (2000), OI | 1.51 | 20.69 |
| Vink et al. (2000), OB | 1.83 | 18.68 |
| Repolust et al. (2004), OI, *cl | 2.00 | 17.98 |
| Markova et al. (2004), O, “case D” | 1.90 | 18.58 |
| Martins et al. (2005), O | 3.15 | 10.29 |
| Mokiem et al. (2005), O, early B | 1.86 | 18.71 |
| Mokiem et al. (2005), O, early B, *cl | 1.58 | 20.16 |
| Mokiem et al. (2007b), O, early B | 1.84 | 18.87 |
| Mokiem et al. (2007b), O, early B, *cl | 1.56 | 20.23 |
Notes. Except for Vink et al., all values have been derived from observational results. Investigated spectral types are provided. The theoretical Vink values refer to the hot side of the bi-stability jump. The values denoted by “*cl” have been derived from mass-loss rates corrected for wind clumping. Units of D0 are in the cgs system.
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