Fig. 7.
Modified wind momentum versus updated luminosity for the Galactic WC & WO stars. The purple-dashed line gives the linear regression fit to these results. For comparison, the relations for OB stars from Kudritzki et al. (1999) and Vink et al. (2000) are shown as gray and black dashed lines. The gray symbols without labels denote the results from Crowther et al. (2002) for the LMC WC4 stars.
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