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Table 1
Selected representative orbits for the 3 d.o.f. Milky Way system given by the potential Eq. (1).
| Orbit | Initial location | (x0,y0,z0), | (Vx0,Vy0,Vz0) | Dominant behaviour | |
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| HF1 | High z, far from centre, low velocity | (10.0,0.0,10.0) | (0.0,50.0,0.0) | Chaotic | |
| HF2 | High z, far from centre, high velocity | (10.0,0.0,10.0) | (0.0,200.0,0.0) | Mainly regular | |
| HC1 | High z, close to centre, low velocity | (5.0,0.0,10.0), | (0.0,50.0,0.0) | Chaotic | |
| HC2 | High z, close to centre, high velocity | (5.0,0.0,10.0) | (0.0,200.0,0.0) | Mainly regular | |
|
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| LF1 | Low z, far from centre, low velocity | (10.0,0.0,0.5) | (0.0,50.0,0.0) | Chaotic | |
| LF2 | Low z, far from centre, high velocity | (10.0,0.0,0.5) | (0.0,200.0,0.0) | Regular | |
| LC1 | Low z, close to centre, low velocity | (5.0,0.0,0.5) | (0.0,50.0,0.0) | Highly chaotic | |
| LC2 | Low z, close to centre, high velocity | (5.0,0.0,0.5) | (0.0,200.0,0.0) | Regular | |
Notes. The dominant behaviour label refers to the intensity of the chaos for most halo parameters.
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