Fig. B.2
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Radial profiles of the surface density results after 1000 inner planet orbits for the resolution used in all the simulations presented in the paper (nr = 540, nϕ = 1024) compared to a higher resolution (nr = 1080, nϕ = 2048). The results are for the dust fluid with a grain size of adust = 5μm with simulation setup VII in both cases.
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