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Fig. 11


Left: the observed (i.e., reddened, in full) and original (i.e., dereddened, in dashed) stellar SED model plotted over the stellar fluxes. The inset shows a zoom-in on the actual measurements. Right: the circumstellar SED (not corrected for reddening), obtained after subtracting the measured total fluxes with the reddened stellar Kurucz model, overplotted with the same reddened Kurucz model (in gray) but with the angular diameter arbitrarily scaled to these circumstellar fluxes. Both panels have the same scales on the x and y axes to illustrate the large amount of circumstellar flux.

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