Direct N-body simulations of Palomar 5 show that no single Milky Way potential model—with or without a bar, flattened halo, LMC, or decelerating bar—reproduces all observed stream properties.
H., Sneden, C., & Kraft, R
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Disentangling the Morphology of Palomar~5: Effects of the Bar, Spiral Arms, LMC, and Halo Flattening
Direct N-body simulations of Palomar 5 show that no single Milky Way potential model—with or without a bar, flattened halo, LMC, or decelerating bar—reproduces all observed stream properties.