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Fig. 5.
Maximum eccentricity (in different colours) during orbital integrations of 12 Myr on the (a0, i0) plane. We show only for i0 ∈ [0 ° ,40 ° ] because there are no stable orbits with i0 > 37°. The black star stands for an orbit of (a0, i0)=(0.9999, 27 ° ) that is shown in Fig. 6.
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