Fig. 7
Logarithmic Eddington fluxes as a function of wavelength for supergiant models (see Tables 1 and 2). The solid lines refer to results from our updated version of FASTWIND and the dashed lines to WM-basic results (Pauldrach et al. 1994, 2001). For clarity, the S35, S40, S45, and S50 model fluxes have been shifted by −3, −6, −9, and −18 dex, respectively.
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