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Fig. 1

image

Spectral energy distributions obtained from the 1D model overlaid on observed flux densities of each source. Peak flux densities in the millimeter range have been adjusted to fit the radial extent of the model. Each caption gives the temperatures of the black body components (top right), the maximum flux Fmax, and the corresponding wavelength of the SED, the flux F12 at 12 μm, and the contribution of the hot part (F35, integrated flux for λ< 35 μm) to the total integrated flux Ftotal (top left).

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