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Fig. 8


The entire SED of the ε Eri dust disk. Symbols with error bars are data points, small dots is the IRS spectrum. Thick line in each panel is the excess emission predicted by the models, and thin lines show contributions from the inner region (<10   AU) and the intermediate + outer disk. Three panels are for the planet configurations “A” (top), “B” (middle), and without a planet (bottom).

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

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