Fig. 8
Mass loss versus luminosity relation with the location of the WO stars. Results for Galactic WC stars from Sander et al. (2012) and LMC WC stars from Crowther et al. (2002) are also indicated. Also plotted are the prediction for WC abundances of Nugis & Lamers (2000) with an additional 
metallicity dependence (Vink & de Koter 2005). The gray symbols indicate the Nugis & Lamers (2000) predictions for the WO stars, which underpredict the observed mass-loss rates.
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