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Table A.4

Initial characteristics of B-type models.

No. M mo q tp Q tp; min Q tp; max β
[ M ] [km] [km] [km] [1]

B1 10-8 500 5 × 103 5 × 104 0.629
B2 10-10 500 5 × 103 5 × 104 0.629
B3 10-12 500 5 × 103 5 × 104 0.629
B4 10-8 103 105 106 0.629
B5 10-8 103 3 × 104 3 × 105 0.629
B6 10-10 103 3 × 104 3 × 105 0.629
B7 10-12 103 105 106 0.629
B8 10-12 103 3 × 104 3 × 105 0.629
B9 10-8 103 104 105 0.07
B10 0.35
B11 0.629
B12 10-8 103 104 105 0.8
B13 0.9
B14 10-9 103 104 105 0.8
B15 0.9
B16 10-10 103 104 105 0.07
B17 0.35
B18 0.629
B19 0.8
B20 0.9
B21 10-11 103 104 105 0.8
B22 0.9
B23 10-12 103 104 105 0.07
B24 0.35
B25 0.629
B26 0.8
B27 0.9

Notes. In all these models, we consider 103 test particles and the massive object moving in the standard orbit having the periastron equal to 0.1 au, apastron 50 au, and initial star-centric distance 5 au. Qtp; min and Qtp; max are the minimum and maximum apocenter distances of test particles orbiting the massive object in a cloud. The other denotations are the same as in Tables A.1 and A.3.

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