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Fig. E.11
Same as Fig. E.1, but for HD 66811 (O4I(n)fp; vsin i = 225 km s-1). The normalisation around H β is imperfect, leading to some slight mismatch between the observation and the fit; the emission of the He ii 4686 line is not reproduced in the model, but we recall that wind parameters were not derived (see Sect. 4.3.2).
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