dSph Satellite Galaxies without Dark Matter: a Study of Parameter Space

dc.creatorKroupa, Pavel
dc.date1998-04-24
dc.date.accessioned2026-07-07T02:26:41Z
dc.date.available2026-07-07T02:26:41Z
dc.descriptionA parameter study is underway in Heidelberg that aims to find and constrain possible solutions to the dSph satellite problem under the assumption that some of these systems may not be dark matter dominated. The present state of the parameter survey of tidally disrupting spheroidal dwarf galaxies is described, and examples of preliminary results are presented.
dc.description4 pages, LaTeX, to appear in the Proceedings of the Bonn/Bochum-Graduiertenkolleg Workshop ``The Magellanic Clouds and Other Dwarf Galaxies'', 18.-22. January 1998, Tom Richtler & Jochen M. Braun (eds.), Shaker Verlag
dc.identifierhttps://arxiv.org/abs/astro-ph/9804255
dc.identifierhttp://arxiv.org/abs/astro-ph/9804255
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12371
dc.subjectAstrophysics
dc.titledSph Satellite Galaxies without Dark Matter: a Study of Parameter Space
dc.typetext

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