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Table 1:

Stellar parameters of studied O stars.

Star
HD Sp. R* M $\mbox{$T_{\rm eff}$ }$ L $\dot M$
    type $[{R}_{\odot}]$ $[{M}_{\odot}]$ $[10^3~{\rm K}] $ $[10^5~{L}_\odot]$ $[\ensuremath{\ensuremath{{M}_{\odot}}/{\rm year}} ]$
$\xi$ Per 24912 O7.5IIIe 14.0 36 35.0 2.64 $4.6\times10^{-7}$
$\alpha$ Cam 30614 O9.5Iae 27.6 43 30.9 6.23 $1.5\times10^{-6}$
$\lambda$ Ori A 36861 O8 III 12.3 30 36.0 2.28 $5.1\times10^{-7}$
$\iota$ Ori A 37043 O9III 21.6 41 31.4 4.07 $6.3\times10^{-7}$
$\zeta$ Ori A 37742 O9Iab 24.0 34 31.5 5.09 $1.5\times10^{-6}$
15 Mon 47839 O7Ve 9.9 32 37.5 1.74 $2.8\times10^{-7}$
  54662 O7III 11.9 38 38.6 2.82 $8.9\times10^{-7}$
  93204 O5V 11.9 41 40.0 3.25 $1.4\times10^{-6}$
$\zeta$ Oph 149757 O9V 8.9 21 32.0 0.75 $4.6\times10^{-8}$
63 Oph 162978 O8III 16.0 40 37.1 4.35 $2.0\times10^{-6}$
68 Cyg 203064 O8e 15.7 38 34.5 3.13 $6.1\times10^{-7}$
19 Cep 209975 O9Ib 22.9 47 32.0 4.93 $8.6\times10^{-7}$
$\lambda$ Cep 210839 O6Iab 19.6 51 38.2 7.34 $6.4\times10^{-6}$
AE Aur 34078 O9.5Ve 7.5 20 33.0 0.60 $1.4\times10^{-8}$
$\mu$ Col 38666 O9.5V 6.6 19 33.0 0.46 $7.8\times10^{-9}$
  42088 O6.5V 9.6 31 38.0 1.72 $3.4\times10^{-7}$
  46202 O9V 8.4 21 33.0 0.75 $2.3\times10^{-8}$

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