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Table A.3.
Initial conditions in the Newtonian simulation
Stars | ||
---|---|---|
Primary | Secondary | |
Profile | Hernquist sphere | Exponential disk |
log10(Mass/M⊙) | 10.521 | 9.82 |
Scale length [kpc] | 2 | 2 |
Exponential scale height [kpc] | – | 0.6 |
Number of particles | 1,400,597 | 278,813 |
DM halos | ||
Primary | Secondary | |
Profile | NFW | NFW |
Characteristic density [M⊙ kpc−3] | 2.76 × 106 | 3.87 × 106 |
Scale radius [kpc] | 31.1 | 17.7 |
Truncation radius [kpc] | 100 | 100 |
log10(Mass/M⊙) | 11.85 | 11.45 |
Number of particles | 5,938,956 | 2,381,632 |
Orbital parameters | ||
(position of secondary) − (position of primary) | (100, 0, 0) kpc | |
(velocity of secondary) − (velocity of primary) | (0, −5.0, 0) km s−1 | |
Spin of secondary | (0, 0, 1) |
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