Fig. 9
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Dynamical maps in the Keplerian, osculating astrocentric semi-major-axis-eccentricity plane for the quasi-periodic, near-resonant configuration described by Model 2. All masses and elements but the map coordinates are fixed at their best-fitting values in Table 7. The osculating epoch is 1998.830. Stable solutions are determined with |〈Y〉 − 2| ≃ 0 and marked with blue color.
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