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Fig. 9
Location of DR1 in the Hertzsprung-Russell Diagram. Also plotted are the WO2 and WC stars analyzed by Sander et al. (2012), the LMC WO3 star analyzed by Crowther et al. (2000) and evolutionary tracks for SMC metallicity from Meynet & Maeder (2005) for an initial rotation rate of 300 km s-1.
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