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Fig. 2.


Pericenter vs. apocenter properties of the galaxies in the sample with 3D velocity errors < 100 km s−1, as indicated by the labels. The top panel plot shows the results for a MW DM halo of virial mass equal to 1.6 × 1012M, and the lower panel for 0.8 × 1012M. We also show typical virial radii in both plots. Gru I is omitted in the lower plot because of the very large apocenter.

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