From streaming instability to the onset of pebble accretion - I. Investigating the growth modes in planetesimal rings

Open Access

Fig. 5

Mass of the largest body in the ring (embryo; solid), the initial characteristic planetesimal mass (dash doted), and ring mass (dotted). The background colours refer to the different pebble accretion regimes (red: ballistic/isolation regime; brown: Bondi regime; and green: Hill regime).

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