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Table 2

Parameters of the sample stars.

Star Spectral Teff log g log gc V sin i vmac He/H C/H N/H O/H
type [kK] [km s-1] [km s-1] [10-4] [10-4] [10-4]

HD 12323 ON9.2 V 33.5 4.00 4.01 130 0.16 <0.3 3.5 2.5
HD 13268 ON9.5 IIIn 32 3.50 3.63 310 0.20±0.10 <0.5 5.0 3.1
HD 14633 ON8.5 V 34 3.80 3.81 100 120 0.13 <0.3 5.2 1.7
HD 48279 ON8.5 V 34.5 3.80 3.82 137 50 0.16±0.05 0.65 4.6 4.3
HD 91651 ON9.5 IIIn 31 3.50 3.62 310 0.14 <0.5 5.4 2.3
HD 102415 ON9 IIInn 31 3.50 3.70 376 0.21±0.10 <0.6 7.6 <3.0
HD 117490 ON9.5 IIInn 30.5 3.50 3.66 375 0.16 <0.3 7.6 2.5
HD 123008 ON9.2 Iab 30 3.10 3.10 37 100 0.21 0.22 13.5 4.8
HD 150574 ON9 III(n) 31 3.40 3.49 240 0.23±0.06 <0.5 >10.0 6.0
HD 191423 ON9 II-IIInn 31.5 3.50 3.72 445 0.25±0.08 >5.0
HD 191781 ON9.7 Iab 28 3.10 3.12 107 70 0.25 <0.5 7.3 3.1
HD 201345 ON9.2 IV 34 4.00 4.01 95 60 0.1 <0.4 4.0 3.6

Notes. Uncertainties on Teff, log g, V sin i  and vmac are ~1.5 kK, 0.15 dex, 10, and 20 km s-1 respectively. log gc is the surface gravity corrected for centrifugal acceleration. Abundances are number ratios.

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