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Fig. 20


Filtering efficiency of a swarm of planetesimals with radii between 1 km and 1000 km as a function of orbital distance and , the mass of the gas disk in MMSN units, for α = 10-2. The panels corresponds to various dust sizes ranging from 1 micron (top) to 10 m (bottom). Within each panel, disk evolution proceeds from top (large ) to bottom (small ). A negative value of Log(xfilter) indicates inefficient filtering. Efficient filtering is shown as white areas.

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