Parametric Dwarf Spheroidal Tidal Interaction

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dc.creatorFleck, Jean-Julien
dc.creatorKuhn, Jeff R.
dc.date2003-02-21
dc.date.accessioned2026-07-07T12:53:39Z
dc.date.available2026-07-07T12:53:39Z
dc.descriptionThe time dependent tidal interaction of the Local Group Dwarf Spheroidal (dS) Galaxies with the Milky Way (MW) can fundamentally affect their dynamical properties. The model developed here extends earlier numerical descriptions of dS-MW tidal interactions. We explore the dynamical evolution of dS systems in circular or elliptical MW orbits in the framework of a parametric oscillator. An analytic model is developed and compared with more general numerical solutions and N-body simulation experiments.
dc.description24 pages, 15 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0302463
dc.identifierhttp://arxiv.org/abs/astro-ph/0302463
dc.identifierAstrophys.J.592:147-160,2003
dc.identifierdoi:10.1086/375585
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223697
dc.subjectAstrophysics
dc.titleParametric Dwarf Spheroidal Tidal Interaction
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