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Table 4.

Assumed stellar parameters for the FASTWIND calculation of the calibrated spectra.

Object ID SpT Teff [K] log L [L] M [M] R [R] [M yr−1] v [km s−1]
HD 93 128 O3.5 V((fc))z 43 854 5.75 52.44 13.11 3.24e–06 3212.75
HDE 319 699 O5 V((fc)) 40 862 5.49 38.08 11.20 1.29e–06 2962.01
HD 124 314 O6 IV(n)((f)) 38 867 5.32 30.98 10.11 6.82e–07 2811.98
HD 150 135 O6.5 V((f))z 37 870 5.23 28.00 9.61 4.77e–07 2741.98
HD 150 135 O8: 34 877 4.96 20.76 8.29 1.55e–07 2542.05
HDE 326 775 O6.5 V(n)((f))z 37 870 5.23 28.00 9.61 4.77e–07 2741.98
V3903 Sgr O7 V(n)z 36 872 5.14 25.29 9.15 3.32e–07 2670.61
V3903 Sgr B0: V 32 020 4.31 15.00 5.10 7.12e–09 2755.87
HD 152 623 O7 V(n)((f)) 36 872 5.14 25.29 9.15 3.32e–07 2670.61
BD −13° 4929 O8 V 34 877 4.96 20.76 8.29 1.55e–07 2542.05
BD −13° 4929 B0.5: V 29 700 5.14 16.00 5.67 2.55e–08 2721.23
HD 149 452 O9 IVn 32 882 4.77 17.08 7.53 6.63e–08 2419.32
HD 76 341 O9.2 IV 32 383 4.72 16.31 7.35 5.24e–08 2392.93
BD −13° 4928 O9.5 V 31 884 4.68 15.55 7.18 4.35e–08 2364.01
CPD −41° 7721 O9.7 V:(n) 31 884 4.68 15.55 7.18 4.35e–08 2364.01
HD 152 200 O9.7 IV(n) 31 385 4.64 14.79 7.00 3.61e–08 2334.97

Notes. Effective temperatures Teff, logarithmic luminosities log L, masses M, and radii R are taken from Martins et al. (2005) and Trundle et al. (2007), for O- and B-type stars, respectively. The mass-loss rate () and terminal wind velocities (v) are computed following the prescriptions given by Vink et al. (2001).

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