Fig. 5

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Spherically symmetric dust geometries used in RADMC-3D, centred on the star. Colour bars show the logarithm of dust density in g cm−3. Top: single continuous shell of dust (S). Middle: continuous dust shell with an overdense shell at the outer edge (D). Bottom: two-shell model with a cavity (CD). The labelled arrows indicate the size parameters used in the model, except for rin, which is unresolved at this resolution.
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