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Fig. 2


Evolution of the mass of a planet of initially 0.1 M accreting pebbles in the B77 DHARP ring, for three different locations (i.e., values of δ) relative to the position of the pressure maximum as well as a case (black curve) where the planet follows the (mass-dependent) location of the planet trap as it grows, and therefore δ changes withtime (from ~0.2 to ~ 0.4).

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