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Fig. E.10
The temperature of VFTS 169 (O2.5 V(n)((f*))) is based on the lines He i λ4471, N iv λ4058, and N v λ4604/4620. Ṁ is based on He ii λ4686. The stellar rotation is high and the model spectrum is convolved with a rotation profile. N-abundance is normal.
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