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Table A.3

Initial characteristics of A-type models with the massive object in orbits other than the “standard orbit” (periastron distance of 0.1 au; apastron distance of 50 au) and/or at distances other than the standard initial star-centric distance (5 au).

No. q Q r o N M mo q tp Q tp β
[au] [1] [ M⋆ ] [km] [km] [1]
A82 1.4 R⋆ 40 1.6 R⋆ 103 10-7 104 105 0.007
A83 0.07
A84 0.629
A85 1.4
A86 1.5 R⋆ 50 5 au 103 10-7 103 105 0.007
A87 0.07
A88 0.629
A89 1.4
A90 1.5 R⋆ 50 5 au 103 10-9 103 105 0.007
A91 0.07
A92 0.629
A93 1.4
A94 1.5 R⋆ 50 1 au 103 10-7 103 104 0.007
A95 0.07
A96 0.629
A97 0.769
A98 1.4
A99 1.5 R⋆ 50 1 au 103 10-7 103 105 0.007
A100 0.07
A101 0.629
A102 1.4
A103 0.1 au 50 3 au 103 10-10 103 105 0.629
A104 1.5 R⋆ 50 1 au 103 10-7 104 105 0.007
A105 0.07
A106 0.629
A107 0.769
A108 1.4
A109 1.5 R⋆ 50 1.5 R⋆ 103 10-7 104 105 0.007
A110 0.07
A111 0.629
A112 1.4
A113 0.05 au 50 5 au 103 10-10 103 104 0.629
A114 0.05 au 50 5 au 103 10-10 103 105 0.629
A115 0.1 au 50 10 au 103 10-11 75 7.5 × 104 0.629
A116 0.1 au 50 10 au 103 10-12 75 7.5 × 104 0.629
A117 0.2 au 15 5 au 103 10-7 103 105 0.629
A118 0.2 au 15 5 au 103 10-10 103 105 0.007
A119 0.629
A120 1 au 50 5 au 103 10-10 103 105 0.07
A121 0.629
A122 0.1 au 50 3 au 103 10-10 103 104 0.629
A123 0.1 au 50 7 au 103 10-10 103 104 0.629
A124 0.1 au 50 10 au 103 10-10 103 104 0.629
A125 1.5 R⋆ 50 5 au 104 10-7 3238 6476 0.07
A126 0.35
A127 0.629
A128 1.5 R⋆ 50 5 au 104 10-8 1503 3006 0.007
A129 0.07
A130 0.35
A131 0.629
A132 1.4 R⋆ 40 1.6 R⋆ 103 10-7 104 vq = 0.1 v ii 0.007
A133 0.07
A134 0.629
A135 1.4 R⋆ 40 1.6 R⋆ 103 10-9 103 vq = 0.1 vii 0.007
A136 0.07
A137 0.629
A138 1.4 R⋆ 40 1.6 R⋆ 103 10-9 103 vq = vii 0.007
A139 0.07
A140 0.629
A141 1.5 R⋆ 50 1 au 103 10-7 104 vq = 0.1 vii 0.007
A142 0.07
A143 0.629
A144 1.5 R⋆ 50 1.5 R⋆ 103 10-7 104 vq = 0.1 vii 0.01
A145 0.07
A146 0.629
A147 1.5 R⋆ 50 1.5 R⋆ 103 10-9 104 vq = 0.1 vii 0.007
A148 0.07
A149 0.629
A150 1.5 R⋆ 50 1.5 R⋆ 103 10-7 104 vq = vii 0.007
A151 0.07
A152 0.629
A153 1.5 R⋆ 50 1.5 R⋆ 103 10-9 104 vq = vii 0.007
A154 0.07
A155 0.629
A156 1.5 R⋆ 50 1.5 R⋆ 103 10-7 104 vq = 10 vii 0.007
A157 0.07
A158 0.629
A159 10 R⋆ 50 5 au 104 10-12 100 103 0.07
A160 1.5 R⋆ 50 5 au 104 10-7 103 105 0.07
A161 0.35
A162 0.629
A163 1.5 R⋆ 50 5 au 104 10-8 103 105 0.007
A164 0.07
A165 0.629
A166 1.5 R⋆ 50 5 au 104 10-10 103 105 0.07
A167 0.35
A168 0.629
A169 2 R⋆ 50 5 au 104 10-8 103 105 0.07
A170 4 R⋆ 50 5 au 104 10-12 100 103 0.07
A171 0.629
A172 1.5 R⋆ 50 5 au 103 10-7 5 × 103 104 0.007
A173 0.07
A174 0.629
A175 1.5 R⋆ 50 5 au 103 10-10 5 × 103 104 0.007
A176 0.07
A177 0.629
A178 1.5 R⋆ 50 5 au 103 10-9 103 104 0.007
A179 0.07
A180 0.629
A181 0.1 au 50 3 au 103 10-10 103 105 0.629
A182 0.05 au 50 5 au 103 10-10 103 105 0.629
A183 0.05 au 50 5 au 103 10-10 103 104 0.629
A184 10 R⋆ 50 5 au 104 10-12 100 103 0.07
A185 0.1 au 15 5 au 103 10-10 103 105 0.07
A186 0.35
A187 0.629

Notes. The periastron and apastron of the massive-object orbit are denoted by q and Q. The initial star-centric distance of this object is denoted by ro and the number of test particles by N. The other symbols are the same as in Table A.1. q and ro are given either in the radii of the central star, R⋆, or in astronomical units. The velocity in the pericenter, vq, with respect to the massive object is given as a multiple of escape velocity from this object, vii.

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