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The Astrophysical Journal
Article . 2003 . Peer-reviewed
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The Astrophysical Journal
Article
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arXiv.org e-Print Archive
Preprint . 2003
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https://dx.doi.org/10.48550/ar...
Article . 2003
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https://dx.doi.org/10.1086/375...
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Parametric Dwarf Spheroidal Tidal Interaction

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 20 Jul 2003Embargo end date: 01 Jan 2003 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 592, pages 147-160 (issn: 0004-637X, eissn: 1538-4357, Copyright policy )
Authors: Fleck, Jean-Julien; Kuhn, Jeff R.;

doi: 10.1086/375585 , 10.48550/arxiv.astro-ph/0302463

arXiv: astro-ph/0302463

Parametric Dwarf Spheroidal Tidal Interaction

Abstract

The 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.

24 pages, 15 figures

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
30
Top 10%
Top 10%
Top 10%
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