Fig. 4
Relative velocity between the planet and pebbles (dark blue line) and number of accreted pebbles (light blue bars) as function of the planet’s orbital phase angle. Perihelion is at 0° and aphelionis at 180°. The planet eccentricity is ep = 0.007 in the left panel and ep = 0.03 in the right panel. Other parameters are the same for the two panels: Mp = 0.01 M⊕, M⋆ = 1 M⊙, τs = 10−2, vhw = 60 m s−1 and Ntot = 300 × 300. The black dashed line represents the transition velocity from the settling to the ballistic accretion, v = v* (Eq. (13)).
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