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Table 6
Stellar parameters derived from the fastwind analysis for the stars that are too hot to derive abundances.
| Name | Spectral | vsini | vmac | vrad | Teff | log g | YHe | ξ | log Q |
| type | (km s-1) | (km s-1) | (km s-1) | (kK) | (dex) | (km s-1) | |||
|
|
|||||||||
| S15 | O7.5 V | 105 | 40 | 36 | 38.8 ± 0.8 | >4.16 | <0.10 | 5 | <–13.5 |
| S17 | O7 Vz | 140 | 0 | 45 | 38.1 ± 1.0 | 4.1 ± 0.2 | 0.12 ± 0.02 | 5 | <–13.5 |
| S33 | O6 V((f)) | 53 | 76 | 48 | 40.0 ± 1.0 | 3.9 ± 0.1 | 0.11 ± 0.02 | 10 | −12.8 ± 0.2 |
| HD 292163 | O8 Vz+ | 35 | 0 | 4 (var) | 39.2 ± 0.8 | >4.2 | 0.20 ± 0.05 | 5 | <–13.5 |
| HD 292090 | ~O8 V | 280 | 0 | 4: | 36.6 ± 2.8 | 3.9 ± 0.4 | 0.1 ± 0.1 | 10 | −13.3 |
| HD 292392 | O8.5 V | 280 | 0 | 29 | 35.8 ± 2.3 | 3.9 ± 0.4 | 0.21 ± 0.09 | 10 | −12.8 ± 0.2 |
| HD 292167 | O8.5 Ib((f)) | 150 | 0 | 31 | 32.6 ± 1.7 | 3.3 ± 0.2 | 0.12 ± 0.04 | 10 | −12.3 ± 0.1 |
Notes. The typical uncertainty for ξ is 2 km s-1.
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