Fig. 4.
Properties of Crater II. Top: orbital integration for Cra II in the MWpotential14 for the standard light halo (blue line) and the heavy DM halo (red line) plotted as the distance from the MW center as a function of time. Bottom: hill radius of a galaxy of the mass of Cra II (Caldwell et al. 2017) in two different MW potentials compared to the size and apocenter of Cra II.
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