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Table 5

Stellar parameters obtained from the optical analysis using unclumped models.

Star Spectral type Teff [kK] log g [dex] log Q YHe υmic [km s−1] ß
HD 46223 O4V((f)) 43.0 ± 1.2 3.76 ± 0.07 −12.8 ± 0.2 0.10 ± 0.03 >9.1 1.0 ± 0.2
HD 15629 O4.5 V((fc)) 41.4 ± 1.4 3.71 ± 0.11 −12.7 ± 0.2 0.12 ± 0.03 <19.9 1.0 ± 0.2
HD 46150 O5 V((f))z 41.2 ± 1.0 3.78 ± 0.07 −13.0 ± 0.3 0.09 ± 0.03 >5.0 >0.8
HD 217086 O7 Vnn((f))z 37.0 ± 1.0 3.60 ± 0.11 −13.9 ± 1.1 0.11 ± 0.03 12.4 ± 7.4 <1.2
HD 149757 O9.2 IVnn 32.5 ± 0.9 3.84 ± 0.17 −14.1 ± 0.9 0.11 ± 0.03 12.2 ± 7.2 <1.2
HD 190864 O6.5 III(f) 37.1 ± 0.7 3.58 ± 0.05 −12.7 ± 0.1 0.12 ± 0.03 15.1 ± 3.4 0.9 ± 0.1
HD 203064 O7.5 IIIn((f)) 34.9 ± 0.7 3.54 ± 0.11 −12.7 ± 0.1 0.10 ± 0.03 >15.2 0.9 ± 0.1
HD 15570 O4 If 40.1 ± 0.9 3.75 ± 0.18 −12.0 ± 0.1 0.11 ± 0.03 >5.0 >1.0
HD 14947 O4.5 If 38.1 ± 0.5 3.61 ± 0.05 −12.0 ± 0.1 0.15 ± 0.03 >9.5 >1.2
HD 30614 O9 Ia 29.4 ± 0.8 2.96 ± 0.09 −12.2 ± 0.1 0.14 ± 0.03 >15.9 >0.8
HD 210809 O9 Iab 31.1 ± 0.3 3.17 ± 0.07 −12.4 ± 0.1 0.12 ± 0.03 >16.2 >1.0
HD 209975 O9.5 Ib 31.3 ± 0.4 3.23 ± 0.05 −12.7 ± 0.1 0.10 ± 0.03 >12.2 >1.1

Notes. Gravities do not include a centrifugal correction. Upper and lower limits refer to the corresponding parameter ranges of our model grid only (see Table 2).

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