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Fig. E.5
He i λ4471 is too broad for VFTS 094 (O3.5 Inf*p + sec) possibly as a result of its status as a SB2. The fit quality is reasonably good for a SB2, but the luminosity is uncertain as the contribution of the secondary is unknown. N and He are enriched at the surface. The star is evolved with Hα and He ii λ4686 in emission.
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