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Effect of the Magellanic Clouds on the Milky Way Disk and VICE VERSA
Astronomy Department Faculty Publication Series
  • Martin D. Weinberg, University of Massachusetts - Amherst
Publication Date
1998
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This paper was harvested from ArXiv identifier is arXiv:9811204v1
Abstract

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.

Citation Information
Martin 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/