Fig. E.1.
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Observed spectra and photometry of MWC 656 (blue) compared to composite model fits (red). The models combine the rapidly rotating Be star (brown) with a stripped companion (green). The example shown here assumes a cooler stripped star (T* = 65 kK) than in the fiducial best-fit model (T* = 85 kK). Cooler models strengthen C IV and over-predict the emission in He II.
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