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Fig. 13


Variation in distance d0.5 with the dark halo flattening, qz. The orientation is fixed to φ = 90. Left: variation in the L-orbits, close to disc orbits. Right: variation in the H-orbits, orbits with higher z. The L-orbits show the higher values. The H-orbits show the lowest values, but they are never low enough to produce low predictabilities.

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