Fig. 3

Top: radial profile of the gas surface density for our reference model MREF. The steep rise at around 0.11 au is due to the drop in the accretion stress. Bottom: profile of the midplane scale height H/R. The markings in the panels show the values at 1 au (dotted lines), the position of the pebble trap (black cross, ×) and typical slope profiles for comparison (black lines).
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