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Fig. 9


Dereddened SED of TYC 3683-985-1 from optical to infrared wavelengths (dashed line) built from the UJT magnitudes in the maximum and far-infrared data from the WISE bands (Wright et al. 2010). The thick line has been plotted for comparison purposes. It corresponds to a Kurucz model for an isolated B3V star normalised to the B-band emission level where the free-free excess from the circumstellar disc is almost negligible.

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