Fig. 9
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Mass-loss rate (log Ṁ) vs. bolometric luminosity (log L⋆) for the O-type stars analyzed in N11 B. In addition, the stars Sk −66° 171 and Sk −69° 50 (not in N11 B) are also shown as references (green squares), as well as N11 046 (blue square). An increasing trend between M and log L⋆ is observed. Notations are the same as in Fig. 8. Typical uncertainties are indicated.
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