Fig. 6

Phased time series spectra around Hα line folded with the orbital period of the system and corresponding Doppler maps. The orbital period of Porb = 84.1 days, the primary mass of M1 = 14.0 M⊙, and the mass ratio of q = 0.16 are used to overlay positions of the stellar components on the Doppler maps. The inclination angle i = 70° is arbitrarily chosen based on suggestions by Bjorkman et al. (2002). φorb = 0.0 corresponds to the inferior conjunction of the secondary.
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