Open Access

Fig. 3

image

Column density of different populations is displayed against R for several snapshots. Top left panel: primordial dust, top right, bottom left and bottom right: primordial pebbles, planetesimals and collisional dust, respectively. We depict a combined result of multiple 0-d simulations executed at 20 different radii to allow an insight in a possible global evolution of the dust profile. All simulations shown in this figure used ɛ = 0.01.

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