Fig. 5.
Empirical mass-loss rates versus updated luminosity for the Galactic WC & WO stars. The red-dashed line gives the linear regression fit to these results. The relations proposed by Nugis & Lamers (2000) for WC stars with 40% and 60% carbon, respectively, are indicated by the thick and thin shaded lines. The results from Crowther et al. (2002) for the LMC WC4 stars are denoted by gray symbols.
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