Fig. E.50
The temperature of VFTS 682 (WN5h) is based on the lines N iv λ4058, N v λ4604/4620, and on the absence of the He i λ4471 line. Ṁ and He-abundance are based on He ii λ4686 and Hα. The fit quality is reasonably good for a WNh stars. Even though the best fitting grid model has a slightly too high Ṁ. The results are similar to those from Bestenlehner et al. (2011).
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