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Fig. 5

Fig. 5 Refer to the following caption and surrounding text.

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Evolution of the orbital plane at r = 23.9 au in the retrograde simulation in Configuration 2 (see Figure 2, right). We started the fit according to Equation (3) (blue dashed line) at the first maximum of the curve (dashed gray line) and stopped the fit at t = 1.58 × 104 yr, where the period seems to change. We note that this figure shows the evolution over a longer time period than Figure 3.

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