Flat rotational curves without dark matter

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dc.creatorPronko, G.
dc.date2006-11-09
dc.date.accessioned2026-07-07T07:30:45Z
dc.date.available2026-07-07T07:30:45Z
dc.descriptionWe consider the singular configurations of gravitating gas [1] which could be used as a model for disk galaxies. The simplest steady configuration, which corresponds to rotation of stars around center gives flat rotational curve, provided the density distrubution has a tail, decaying as 1/r. This result based exclusively on Newtonian gravity and does not involve dark matter.
dc.description10 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0611303
dc.identifierhttp://arxiv.org/abs/astro-ph/0611303
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118507
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleFlat rotational curves without dark matter
dc.typetext

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