The satellite-disk interaction provides limits on halo properties in two ways: (1) physical arguments motivate the excitation of observable Galactic disk structure in the presence of a massive halo, although precise limits on halo parameters are scenario-dependent; (2) conversely, the Milky Way as a whole has significant dynamical effect on LMC structure and this interaction also leads to halo limits. Together, these scenarios give strong corroboration of our current gravitational mass estimates and suggests a rapidly evolving LMC.
Weinberg, Martin D., "Effect of the Magellanic Clouds on the Milky Way Disk and VICE VERSA" (1998). Astronomy Department Faculty Publication Series. 25.
Retrieved from https://scholarworks.umass.edu/astro_faculty_pubs/25