Tidal Stream Morphology as an Indicator of Dark Matter Halo Geometry: the Case of Palomar 5
Sarah Pearson, Andreas H. W. K\"upper, Kathryn V. Johnston, Adrian M., Price-Whelan

TL;DR
This study demonstrates that the morphology of the Palomar 5 stellar stream can be used to distinguish between spherical and triaxial dark matter halo models, providing a new method to infer halo geometry without velocity data.
Contribution
It introduces a novel approach to constrain dark matter halo shape using the morphology of a single stellar stream, specifically ruling out a triaxial potential model based on observed stream features.
Findings
Spherical halo models fit Pal 5 stream morphology.
Triaxial potential models cannot reproduce the observed stream curvature.
Stream morphology can indicate dark matter halo triaxiality.
Abstract
This paper presents an example where the morphology of a single stellar stream can be used to rule out a specific galactic potential form without the need for velocity information. We investigate the globular cluster Palomar5 (Pal 5), which is tidally disrupting into a cold, thin stream mapped over 22 degrees on the sky with a typical width of 0.7 degrees. We generate models of this stream by fixing Pal 5's present-day position, distance and radial velocity via observations, while allowing its proper motion to vary. In a spherical dark matter halo we easily find models that fit the observed morphology. However, no plausible Pal 5 model could be found in the triaxial potential of Law & Majewski (2010), which has been proposed to explain the properties of the Sagittarius stream. In this case, the long, thin and curved morphology of the Pal5 stream alone can be used to rule out such a…
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