Fig. B.1.
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The orbit of the satellites that are in interaction with CR-11, CR-12, CR-18 and CR-20, respectively. Each column of panels is constrained to the lookback time window that has a peak in the SFH fo the CRD according to Fig. 9. 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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