Fig. 4

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Delayed eccentricities (top row), inclinations (middle), and semi-major axis (bottom row) for all simulations in the 3:2-3:2 (left column) and 2:1-2:1 (right column) resonant chains. Colors indicate the pericentric distance q between the stars during the flyby event, with each color corresponding to a specific q, while the symbols represent the inclination β of the flyby star. The black dashed line indicates the stability limit given by the orbit-crossing value ecross.
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