Effect of the Magellanic Clouds on the Milky Way Disk and VICE VERSAAstronomy Department Faculty Publication Series
AbstractThe 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.
Citation InformationMartin D. Weinberg. "Effect of the Magellanic Clouds on the Milky Way Disk and VICE VERSA" (1998)
Available at: http://works.bepress.com/martin_weinberg/4/