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Fig. 6
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Initial pebble accretion rate onto a protoplanet as a function of its position and mass. The separation between 3D and 2D accretion regimes and between Bondi and Hill regimes are indicated. In the outer regions, we need to consider 3D and 2D as well as Bondi and Hill regimes. Employed fiducial values are listed in Table 1.
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