Table 5
Fundamental parameters for the early O-star sample, assuming unclumped mass-loss.
Star | Spectral type | Nitrogen | Teff | log g | log gtrue | R ∗ | log L ∗ | Ṁc | log Q | β | v ∞ | vsini | v mac | Y He | [N] |
Teff diag. | (kK) | (cgs) | (cgs) | (R⊙) | (L⊙) | (km s-1) | (km s-1) | (km s-1) | |||||||
|
|||||||||||||||
Dwarfs | |||||||||||||||
BI253a | O2 V((f∗)) | N iv/N v | 54.8 | 4.18 | 4.20 | 10.7 | 5.97 | 1.53 | –12.61 | 1.21 | 3180 | 230 | – | 0.08 | 7.90 |
BI237a | O2 V((f∗)) | N iv/N v | 53.2 | 4.11 | 4.12 | 9.7 | 5.83 | 0.62 | –12.98 | 1.26 | 3400 | 140 | – | 0.09 | 7.38 |
R136-040 | O2-3.5 V | – | > 51.0 | 4.01 | 4.02 | 10.3 | 5.81 | 1.93 | –12.53 | 0.80 | 3400 | 120 | – | 0.08 | 6.90 |
N11-060a | O3 V((f∗)) | N iii/N iv/N v | 48.0 | 3.97 | 3.97 | 9.5 | 5.63 | 0.51 | –12.92 | 1.26 | 2740 | 68 | 40 | 0.12 | 8.20 |
N iv/N v | 51.0 | 4.10 | 4.10 | 9.2 | 5.71 | 0.48 | –12.92 | 8.15 | |||||||
AV 435b | O3 V((f∗)) | N iii/N iv | 46.0 | 3.90 | 3.91 | 13.8 | 5.88 | 0.21 | –13.15 | 0.80 | 1500 | 110 | – | 0.10 | 7.58 |
LH 81:W28-23 | O3.5 V((f+)) | N iii/N iv/N v | 47.0 | 3.80 | 3.82 | 10.0 | 5.65 | 1.57 | –12.53 | 1.00 | 3050 | 146 | – | 0.25 | 8.40 |
LH 101:W3-24 | O3.5 V((f+)) | – | 47.0 | 4.00 | 4.01 | 8.1 | 5.46 | 0.27 | –13.00 | 0.80 | 2400 | 120 | – | 0.10 | 7.78 |
LH 81:W28-5 | O4 V((f+)) | N iii/N iv/N v | 44.0 | 3.80 | 3.81 | 9.8 | 5.51 | 1.08 | –12.60 | 0.80 | 2700 | 120 | 80 | 0.15 | 8.38 |
AV 177b | O4 V((f)) | – | 44.0 | 3.80 | 3.85 | 8.8 | 5.42 | 0.23 | –13.19 | 0.80 | 2650 | 220 | – | 0.15 | 7.78 |
|
|||||||||||||||
Giants | |||||||||||||||
N11-031a | ON2 III(f∗) | N iii/N iv | 47.8 | 3.95 | 3.95 | 13.4 | 5.92 | 2.02 | –12.64 | 1.08 | 3200 | 71 | 60 | 0.11 | 7.83 |
N iv/N v | 56.0 | 4.00 | 4.00 | 12.2 | 6.12 | 2.20 | –12.54 | 8.30 | |||||||
NGC 346-355b | ON2 III(f∗) | N iv/N v | 55.0 | 4.00 | 4.01 | 12.0 | 6.08 | 2.50 | –12.39 | 0.80 | 2800 | 140 | – | 0.10 | 8.10 |
N iii/N iv | 51.0 | 4.00 | 12.5 | 5.98 | 2.00 | –12.51 | – | 7.98 | |||||||
N11-026a | O2 III(f∗) | N iii/N iv/N v | 49.0 | 4.00 | 4.00 | 11.3 | 5.82 | 1.56 | –12.63 | 1.08 | 3120 | 72 | 60 | 0.10 | 7.80 |
N iv/N v | 52.0 | 4.10 | 4.10 | 11.0 | 5.89 | 1.49 | –12.63 | 7.75 | |||||||
R136-018 | O3 III(f∗) | N iii/N iv/N v | 47.0 | 3.90 | 3.92 | 14.2 | 5.95 | 1.68 | –12.76 | 0.80 | 3200 | 180 | – | 0.10 | 8.18 |
LH 90:ST 2-22 | O3.5 III(f+) | N iii/N iv/N v | 44.0 | 3.70 | 3.71 | 18.8 | 6.08 | 4.56 | –12.36 | 0.80 | 2560 | 120 | 80 | 0.15 | 8.58 |
|
|||||||||||||||
Supergiants | |||||||||||||||
Sk–67° 22 | O2 If∗/WN5 | N iii/N iv/N v | 46.0 | 3.70 | 3.74 | 12.4 | 5.80 | 15.00 | –11.60 | 0.80 | 2650 | 200 | – | 0.30 | 8.78 |
LH 101:W3-19 | O2 If∗ | N iii/N iv/N v | 44.0 | 3.90 | 3.91 | 25.3 | 6.34 | 20.86 | –11.97 | 0.80 | 2850 | 180 | – | 0.10 | 8.18 |
Sk–65° 47 | O4 If | N iii/N iv | 40.5 | 3.60 | 3.62 | 19.8 | 5.98 | 11.00 | –11.89 | 0.80 | 2100 | 160 | – | 0.12 | 7.78 |
Notes. log gtrue is the surface gravity corrected for centrifugal effects. For each star, the additional (or even primary) Teff diagnostics used in parallel with the He i/He ii ionization equilibrium is indicated. For four stars, two parameter sets are provided, because we had problems to reach a simultaneous fit for all considered lines from three nitrogen ionization stages. For N11-026 and N11-060 the first entry is our preferred one, and the second entry is a (disfavored) alternative, whereas for N11-031 (see Paper II) and NGC 346-355 we consider both solutions as possible. For errors, see text.
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