Extended Data Fig. 8: Predicted response of the Galactic halo to the LMC.
From: All-sky dynamical response of the Galactic halo to the Large Magellanic Cloud
The N-body simulation presented in Fig. 1b is shown here without any selections, either in proper motions or on-sky (the density profile is still matched to the data, and only stars with 60 < Rgal < 100 kpc are included). a, Projection in the usual Galactic coordinates. b, Projection in Galactocentric coordinates (what an observer would see if placed at the Galactic Centre). In b, the model amplitude of the collective response is asymmetric and is largest near the Galactic plane.
