Fig. 12.
From top to bottom: semi-major axis and eccentricity of the inner (red solid line) and outer binary (black dotted line) for the triple shown in the bottom panel of Fig. 11. The system shows a bound triple in the first ∼4000 yr, then one object marked with light blue is ejected on a weakly bound eccentric orbit, and is ultimately completely ejected on an unbound trajectory.
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