Fig. 14
Spectral energy distribution of the infrared emission in the central part of Ou4. Diamonds and triangles are IRIS and WISE data points, obtained from aperture photometry (Fig. 13). Grey lines show the transmission profiles of the IRAS and WISE broad-band filters, with vertical dotted lines indicating the effective wavelength. The solid line is the dust emission (single-temperature modified black-body model) fitted to the IRIS data points (diamonds), and asterisks are the corresponding modelled fluxes in each filter. The dashed line is the corresponding black-body model.
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