Accretion of eroding pebbles and planetesimals in planetary envelopes

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Table 1

Simulations parameters.

Planet radius	Semi-major axis	Gas pressure at
		planetary surface
R_planet [R_Earth]	a [AU]	p_surface [Pa]
0.1	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

0.2	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

0.3	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

0.5	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

1	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

2	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

3	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

5	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

10	0.1, 0.2, 0.3, 0.5,	0
	1, 2, 3

1	0.1, 0.2, 0.3, 0.5,	10³
	1, 2, 3

1	0.1, 0.2, 0.3, 0.5,	10⁵
	1, 2, 3

Nostes. For each simulation run the pebble size is varied between 10⁻³ and 10⁴ m and the range for the initial y-position is kept largeenough so that all accretion events are considered in the simulations.

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