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Table 2.

Stellar mass-loss rates of O type stars collected from the literature.

HD Name SpT (M yr−1) Ref.
Luminosity class I

HD 66811 O4I 2.5e–6 1
HD 16691 O4I 3.0e–6 2
HD 190429A O4If 2.1e–6 2
HD 15570 O4I 2.8e–6 1
HD 14947 O4.5If 2.8e–6 1
HD 210839 O6.5I 1.6e–6 1
HD 163758 O6.5I 1.6e–6 2
HD 192639 O7.5I 1.3e–6 1

Luminosity class II–III

HD 93250 O4III 5.6e–7 3
HD 15558 O4.5III 1.9e–6 4
HD 190864 O6.5III 4.6e–7 4
HD 34656 O7II 3.0e–7 4
HD 24912 O7.5III 4.0e–7 4
HD 36861 O8III 3.0e–7 4
δ Ori Aa1 O9.5II 4.0e–7 5

Luminosity class V

HD 46223 O4V 3.2e–7 3
HD 15629 O4.5V 3.2e–7 3
HD 93204 O5.5V 1.8e–7 3
HD 42088 O6V((f))z 1.0e–8 3
HD 152590 O7.5Vz 1.6e–8 3
HD 93028 O9IV 1.0e–9 3
HD 46202 O9.2V 1.3e–9 3
HD 38666 O9.5V 3.0e–10 3
HD 34078 O9.5V 3.0e–10 3
HD 36512 O9.7V 5.0e–10 6

Notes. An interested reader is strongly encouraged to consult original papers for details of the spectroscopic analyses.

References. (1) Šurlan et al. (2013); (2) Bouret et al. (2012); (3) Martins et al. (2005a); (4) Repolust et al. (2004), note that the mass-loss rates in the table are reduced by a facor of 3; (5) Shenar et al. (2015); (6) Shenar et al. (2017).

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