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Effect of the Magellanic Clouds on the Milky Way disk and VICE VERSA | | Martin D. Weinberg
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12 Nov 1998 | | Subject: | astro-ph | | Affiliation: | University of Massachusetts/Amherst | | 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. | | Source: | arXiv, astro-ph/9811204 | | Services: | Forum | Review | PDF | Favorites | |
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