Fig. E.1
VFTS 016 (O2 III-If*) is a known runaway (Evans et al. 2010). The temperature is based on the lines N iv λ4058, N v λ4604/4620, and on the absence of He i λ4471. Ṁ is based on the line shape of He ii λ4686. The blue wing of He ii λ4686 and the red wing of Hα is not properly reproduced by the model. However, the stellar parameters are in agreement with Evans et al. (2010).
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