Quantifying the Impact of the Large Magellanic Cloud on the Structure of the Milky Way’s Dark Matter Halo Using Basis Function Expansions

@article{GaravitoCamargo2021QuantifyingTI,
  title={Quantifying the Impact of the Large Magellanic Cloud on the Structure of the Milky Way’s Dark Matter Halo Using Basis Function Expansions},
  author={Nicol{\'a}s Garavito-Camargo and Gurtina Besla and Chervin F. P. Laporte and Adrian. M. Price-Whelan and Emily C. Cunningham and Kathryn V. Johnston and Martin D Weinberg and Facundo A. G{\'o}mez},
  journal={The Astrophysical Journal},
  year={2021},
  volume={919}
}
Indications of disequilibrium throughout the Milky Way (MW) highlight the need for compact, flexible, non-parametric descriptions of phase–space distributions of galaxies. We present a new representation of the current dark matter (DM) distribution and potential derived from N-body simulations of the MW and Large Magellanic Cloud (LMC) system using basis function expansions (BFEs). We incorporate methods to maximize the physical signal in the representation. As a result, the simulations of 108… 
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