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Table 2
Comparison between fits to wind momenta of SMC and LMC OB stars according to Mokiem et al. (2007b) using optical spectroscopy with wind velocities largely estimated from vesc scaling relations, plus this study, for OB stars with dense winds (log Q ≥ −13.2), plus empirical wind velocities.
| log D0 | x | N | Sample | Ref |
|---|---|---|---|---|
| SMC | ||||
| 18.20 ± 1.09 | 1.84 ± 0.19 | 28 | O2–B1 | Mokiem et al. (2007b) |
| 14.78 ± 1.33 | 2.38 ± 0.24 | 26 | OB stars | This study |
| LMC | ||||
| 17.88 ± 0.91 | 1.96 ± 0.16 | 38 | O2–B0.7 | Mokiem et al. (2007b) |
| 15.29 ± 1.14 | 2.32 ± 0.20 | 58 | OB stars | This study |
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