The outcome of collisions between gaseous clumps formed by disk instability

Open Access

Table A.2

Summary of the collision outcomes from all performed simulations

Colliding clumps	N_simulation	N_PM	N_erosion	N_disruption	N_PHR	N_EHR	N_collapse
3M_J young – 3M_J young	38	11	13	6	5	3	0
5M_J evolved – 5M_J evolved	24	1	5	2	6	3	7
10M_J evolved – 1M_J evolved	21	0	0	0	6	0	15
10M_J evolved – 3M_J young	20	0	8	0	1	0	11
10M_J evolved – 5M_J evolved	25	1	0	0	7	0	17
10M_J mid – 5M_J mid	41	8	9	4	7	2	11
10M_J mid – 10M_J mid	33	6	4	1	8	2	12
10M_J evolved – 10M_J evolved	49	2	9	3	15	5	15

Notes. List of pair of colliding clumps with the number of simulations run and the occurrence of each type of outcome, respectively perfect mergers, erosions, disruptions, perfect hit-and-runs, erosive hit-and-runs and collisions resulting in dynamical collapse.

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