Fig. 19
Wind-momentum rates for our sample stars, as a function of log (L/L⊙). Asterisks correspond to supergiants, crosses to other luminosity classes. The two weak wind candidates HD 76341 and HD 37468 are denoted by large symbols. The solid line shows the theoretical predictions for the WLR by Vink et al. (2000), whilst the dashed one has been shifted to lower values by 0.55 dex (see text).
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