Effect of the Magellanic Clouds on the Milky Way disk and VICE VERSA
| dc.creator | Weinberg, Martin D. | |
| dc.date | 1998-11-12 | |
| dc.date.accessioned | 2026-07-07T02:29:05Z | |
| dc.date.available | 2026-07-07T02:29:05Z | |
| dc.description | 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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9811204 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9811204 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13332 | |
| dc.subject | Astrophysics | |
| dc.title | Effect of the Magellanic Clouds on the Milky Way disk and VICE VERSA | |
| dc.type | text |