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Fig. 7


Spectral energy distributions of those 17 objects for which we could determine fluxes in at least four bands overall. Filled circles mark the input fluxes. The black line shows the best fit, and the grey lines show subsequent good fits. The dashed line represents the stellar photosphere corresponding to the central source of the best-fitting model, as it would appear in the absence of circumstellar dust (but including interstellar extinction).

This figure is made of several images, please see below:

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