Extended Data Fig. 9: Predicted density distribution of a tilted stellar halo.
From: All-sky dynamical response of the Galactic halo to the Large Magellanic Cloud
All-sky density distribution of a smooth triaxial model stellar halo that is tilted by 60° along the y axis. While this model captures some of the qualitative behaviour seen in the data (Fig. 1a), it fails to reproduce both the detailed shape of the local wake and predicts a precise symmetry in the north and south, which is not observed.
