Table A.1
Initial characteristics of A-type models with 1000 test particles and the massive object in “standard orbit” (periastron distance of 0.1 au; apastron distance of 50 au) as well as in the standard initial star-centric distance (5 au).
No. | Mmo | qtp | Qtp | β |
[ M⋆ ] | [km] | [km] | [1] | |
|
||||
A1 | 10-10 | 103 | 105 | 0.007 |
A2 | 0.07 | |||
A3 | 0.35 | |||
A4 | 0.629 | |||
A5 | 10-12 | 103 | 105 | 0.007 |
A6 | 0.07 | |||
A7 | 0.35 | |||
A8 | 0.629 | |||
A9 | 10-13 | 103 | 105 | 0.007 |
A10 | 0.07 | |||
A11 | 0.35 | |||
A12 | 0.629 | |||
A13 | 10-14 | 103 | 105 | 0.007 |
A14 | 0.07 | |||
A15 | 0.35 | |||
A16 | 0.629 | |||
A17 | 10-8 | 103 | 105 | 0.000007 |
A18 | 0.007 | |||
A19 | 0.07 | |||
A20 | 0.35 | |||
A21 | 0.629 | |||
A22 | 10-11 | 100 | 100 | 0.629 |
A23 | 10-11 | 100 | 103 | 0.629 |
A24 | 10-12 | 100 | 104 | 0.629 |
A25 | 10-8 | 100 | 105 | 0.629 |
A26 | 10-9 | 100 | 105 | 0.629 |
A27 | 10-10 | 100 | 105 | 0.629 |
A28 | 10-11 | 100 | 105 | 0.629 |
A29 | 10-12 | 100 | 105 | 0.629 |
A30 | 10-11 | 100 | 500 | 0.629 |
A31 | 10-11 | 100 | 5 × 104 | 0.629 |
A32 | 10-9 | 50 | 105 | 0.629 |
A33 | 10-8 | 75 | 7.5 × 104 | 0.8 |
A34 | 10-8 | 0.9 | ||
A35 | 10-9 | 75 | 7.5 × 104 | 0.8 |
A36 | 10-9 | 0.9 | ||
A37 | 10-10 | 75 | 7.5 × 104 | 0.8 |
A38 | 10-10 | 0.9 | ||
A39 | 10-11 | 75 | 7.5 × 104 | 0.629 |
A40 | 10-11 | 0.8 | ||
A41 | 10-11 | 0.9 | ||
A42 | 10-12 | 75 | 7.5 × 104 | 0.8 |
A43 | 10-12 | 0.9 | ||
A44 | 10-12 | 103 | 106 | 0.007 |
A45 | 0.07 | |||
A46 | 0.629 | |||
A47 | 1.4 | |||
A48 | 10-10 | 103 | 104 | 0.35 |
A49 | 0.629 | |||
A50 | 10-10 | 103 | 105 | 1.4 |
A51 | 10-12 | 103 | 105 | 1.4 |
A52 | 10-7 | 103 | 105 | 0.007 |
A53 | 0.07 | |||
A54 | 0.629 | |||
A55 | 1.4 | |||
A56 | 10-8 | 103 | 105 | 1.4 |
A57 | 10-10 | 103 | 1.1 × 103 | 0.629 |
A58 | 10-10 | 103 | 3 × 103 | 0.829 |
A59 | 10-12 | 103 | vq = 300 | 0.007 |
A60 | 0.07 | |||
A61 | 0.629 | |||
A62 | 1.4 |
Notes. Symbols used: Mmo− mass of the MO, qtp and Qtp− pericenter and apocenter distance of the test particles with respect to the MO, and β− parameter characterizing the strength of the Poynting-Robertson drag. In models A59−A62, MO-centric velocity of the particles in the pericenter, vq, is given (in m s-1) instead of Qtp.
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