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Fig. 10.

Fig. 10. Refer to the following caption and surrounding text.

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Orbit of the satellite that continues its interaction with CR-0 at z = 0. We followed the evolution of the satellite orbit to a lookback time of 6 Gyr. Top panel: Evolution of the satellite galactocentric distance from the host. Bottom panel: Evolution of the angle between the angular momentum of the disk and the satellite’s orbital angular momentum. Orbits near 180° are counterrotating, while those near 0° are corotating.

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