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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 ∗  c 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.

(a)

Stellar/wind parameters derived in Paper II;

(b)

SMC star;

(c)

in units of 10-6   M   yr-1.

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