Fig. B.1
Illustration of the effect of the adopted terminal wind speed and clumping factor on the UV and optical spectrum. We show our reference model in black (v∞ = 357 km s-1 and a volume filling factor of 0.5, based on Groh et al. 2008) and compare to a model, for which we adopt values that are typical for WR stars shown in green (v∞ = 1300 km s-1 and volume filling factor 0.1).
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