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Table 2

Fundamental stellar parameters.

Star Sp. type Teff log gc log () β f v ξ t vsin   i Mspec Mevol Age
[kK] [cgs] [km s-1] [M] [M] [Myr]

MPG 355 ON2III(f) 51.7 4.00 6.04 –6.74 0.8 0.02 2800 25 120 64 ± 13.2 >70? ≥3?
AzV177 O4V((f)) 44.5 4.03 5.43 –6.85 1.0 0.05 2400 25 220 31.9 ± 7.2 38.8 1.6
AzV 388 O4V 43.1 4.01 5.54 –7.00 1.3 0.11 2100 20 150 41.4 ± 9.3 42.0 2.2
MPG 324b O4V 42.1 4.00 5.51 –6.85 1.0 0.07 2300 15 70 39.5 ± 9.0 40.0 2.3
MPG 368b O6V 39.3 3.75 5.38 –7.43 1.0 0.10 2100 15 60 26.0 ± 5.9 33.2 3.0
MPG 113 OC6Vz 39.6 4.00 5.15 –8.52 0.8 ... 1250 10 35 24.6 ± 5.6 27.8 2.8
AzV 243 O6V 39.6 3.90 5.59 –7.10 1.0 0.05 2000 15 60 40.8 ± 9.2 41.0 3.0
AzV446c O6.5V 39.7 4.00 5.25 –8.40 0.8 0.10 1400 5 30 28.6 ± 6.5 30.0 3.1
MPG 356 O6.5V 38.2 4.10 4.88 –8.46 0.8 ... 1400 5 20 18.0 ± 4.1 23.1 2.2
AzV 429c O7V 38.3 4.01 5.13 –8.40 0.8 0.10 1300 10 120 26.3 ± 6.0 26.5 3.3
MPG 523 O7Vz 38.7 4.25 4.80 –9.22 0.8 ... 1950 10 50 20.1 ± 4.5 23.1 0.5
NGC346-046 O7Vn 39.0 4.22 4.81 –9.22 0.8 ... 1950 10 300 19.0 ± 4.3 23.7 0.3
NGC346-031 O8Vz 37.2 4.00 4.95 –9.22 0.8 ... 1540 5 25 18.6 ± 4.2 23.2 3.3
AzV 461 O8V 37.1 4.05 5.00 –9.00 0.8 ... 1540 10 200 23.8 ± 5.4 23.8 3.6
MPG 299 O8Vn 36.3 4.25 4.64 –8.52 0.8 ... 1540 5 360 18.3 ± 4.1 19.5 1.5
MPG 487a O8V 35.8 4.00 5.12 –8.52 0.8 .... 1540 2 20 31.7 ± 7.1 25.7 4.3
AzV 267c O8V 35.7 4.04 4.90 –8.60 0.8 0.10 1250 10 220 21.9 ± 5.0 21.5 4.2
AzV 468c O8.5V 34.7 4.00 4.76 –9.15 0.8 ... 1540 5 50 15.7 ± 3.5 19.3 4.3
AzV 148a,c O8.5V 32.3 4.00 4.84 –8.70 0.8 ... 1540 12 60 25.3 ± 5.7 19.0 6.2
MPG 682 O9V 34.8 4.10 4.89 –9.05 0.8 ... 1250 5 40 26.6 ± 6.0 20.8 4.7
AzV 326a O9V 32.4 4.03 4.81 –9.15 0.8 ... 1250 5 200 25.3 ± 5.7 18.8 6.1
AzV 189a O9V 32.3 4.02 4.81 –9.22 0.8 ... 1250 5 150 24.8 ± 5.6 18.8 6.1
MPG 012 B0IV 31.0 3.65 4.93 –9.30 0.8 ... 1250 5 60 17.1 ± 3.9 21.0 6.5

Notes. are given in M yr-1. Evolutionary masses (Mevol) were derived from the tracks by Brott et al. (2011a) (see text for more comments). Uncertainties on Teff are ±1500 K, ±0.1 dex for log g (except AzV 446, AzV 429, AzV 267, AzV 468 and AzV 148, ±0.2 dex), ±0.1 dex on log L/L. As for the wind quantities, an uncertainty of ±0.04 dex was estimated for stars with P Cygni profiles, while v was measured within ±100 km s-1. For stars without P Cygni profiles, see Sect. 3.2 for the procedure we adopted.

(a)

Stars whose photometry was interpreted as indicating binarity (cf. Sect. 5.1).

(b)

Stars showing radial velocity variations (cf. Sect. 5.1).

(c)

Stars whose log g = 4.0 was adopted, because we lacked of optical spectra.

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