What does a typical full disc around a post-AGB binary look like? - Radiative transfer models reproducing PIONIER, GRAVITY, and MATISSE data

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Fig. 3

Same as Fig. 2 but for the dust composition. Top: effect of changing the porosity and the maximum hollow volume ratio assuming the DIANA project opacities. Middle: effect of adding a crystalline component. Bottom: effect of adding a metallic iron component.

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