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Table 3

Summary of the results for the stellar and wind parameters.

Parameter HD 156292 HD 24431 HD 105627 HD 116852 HD 153426 HD 218195 HD 36861 HD 115455 HD 135591
Spectral type O9.7III O9III O9III O8.5II-III((f)) O8.5III O8.5III Nstr O8III O8III((f)) O8IV((f))
log (LL) 5.12 ± 0.20 5.17 ± 0.20 5.17 ± 0.20 5.33 ± 0.20 5.24 ± 0.20 5.24 ± 0.20 5.30 ± 0.20 5.30 ± 0.20 5.10 ± 0.20
                   
(kK) (a) 33.0 ± 3.0 32.0 ± 2.0 33.0 ± 2.0 33.5 ± 2.5 35.0 ± 2.5
                   
(kK) (b) 30.0 ± 2.0 32.5 ± 1.5 35.0 ± 1.0 35.0 ± 1.5 36.0 ± 1.5
                   
log (g) 3.50 ± 0.10 3.75 ± 0.10 3.50 ± 0.10 3.50 ± 0.10 3.55 ± 0.10 3.55 ± 0.10 3.60 ± 0.10 3.57 ± 0.10 3.75 ± 0.10
                   
R (R)
                   
M (M)
                   
v sin i (km s−1) 100 80 160 120 110 80 75 70 80
                   
v (km s−1) 1300 ± 200 2300 ± 300 2100 ± 300 2100 ± 300 2400 ± 300 2000 ± 200 2000 ± 200 2300 ± 300 2100 ± 300

derived (M yr−1) (c)
                   
unclumped (M yr−1) (d)
                   
Vink (M yr−1) (e)
                   
Lucy (M yr−1) (f)

(g)
                   
(e)
                   

Notes. Solar units and g unit are in the cgs system. Modified wind momenta (Dmom) are calculated using the mass-loss rate and terminal velocity in the cgs system and the radius in solar unit. (a) Determined from the UV region (Fe III-IV-V lines). (b)Determined from the optical region (He I-II lines). (c)Mass-loss rate using f = 0.1. (d) unclumped = . (e) Calculated from Vink et al. (2000). (f) Calculated from Lucy (2010a). (g) .

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