Fig. 4
Halo density profile for our chosen model (black line). The best-fit β profile of Miller & Bregman (2013) is shown with a red dashed line, with dotted lines indicating the error in β. The density of the halo determined by the simulations of Gatto et al. (2013) for Carina and Sextans to be stripped in one passage are shown with blue points.
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