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Fig. 1

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Top panels: 2D gas surface density for [1,9,15]    Mjup after 1000 orbits of evolution. Bottom panels: vertically integrated dust-density distribution for each planet mass and for the case of Rp = 20 AU. The white line corresponds to the size of particles that feel the highest radial drift and is proportional to the gas surface density.

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

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