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⊙] | Ṁ [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 (Ṁ) and terminal wind velocities (v∞) are computed following the prescriptions given by Vink et al. (2001).
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