Fig. 7
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Coplanar 1 simulation: same quantities as Fig. 5 for the longer timescale (3000 orbits), corresponding to ~4.9 × 105 yr. The long-time evolution leads to the growth of eccentricity in the disc. Left and centre: gas surface density after 3000 orbits. Right: dust surface density. The dust is still trapped in the gas pressure maximum in an eccentric ring.
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