Fig. 4
Gas and dust distributions in the (r,θ)-plane after 7500 (left panels) and 10 000 (right) yr of evolution. Top row: vertically integrated pressure map of the disc. The rows below show the dust distribution coloured with the logarithm of the Stokes number – from top to bottom panels: 100 μm, 1 mm, 1 cm.Spirals in the gas and in the dust have the same morphology.
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