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Fig. 1

image

SEDs of group Ib Herbig Ae/Be stars in the sample of Maaskant et al. (2014). There is a great similarity in the shape of the SEDs. The fluxes are scaled so that the objects are sorted by dust gap size, with the smallest dust gap radius at the top and the largest dust gap radius at the bottom. The flux scaling factors for the objects from top to bottom are 10, 5, 1, 0.03, 0.003, and 0.003.

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