{
  "id": "astro-ph/9811204",
  "version": "v1",
  "published": "1998-11-12T20:24:14.000Z",
  "updated": "1998-11-12T20:24:14.000Z",
  "title": "Effect of the Magellanic Clouds on the Milky Way disk and VICE VERSA",
  "authors": [
    "Martin D. Weinberg"
  ],
  "comment": "12 pages, 8 Postscript figures, uses paspconf.sty. To appear in the Third Stromlo Symposium: The Galactic Halo (ASP Conference Series), in press. HTML version available at: http://www-astro.phast.umass.edu/~weinberg/stromlo",
  "categories": [
    "astro-ph"
  ],
  "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.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1998-11-12T20:24:14.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "milky way disk",
      "magellanic clouds",
      "vice versa",
      "current gravitational mass estimates",
      "observable galactic disk structure"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 491024
    }
  }
}