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Fig. 9

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Dynamical state of the whole Hungaria group at a given epoch. We used the maximum variations of eccentricity, semi-major axis, and inclination as dynamical indicators. We show the dynamical state of the whole Hungaria group on the ae and aH parameter planes in the right and left panels, respectively. Instead of test particles taken from a regular grid, the orbital elements and absolute magnitudes of real asteroids were used.

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