Linear Potentials in the Cores of Clusters of Galaxies

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dc.creatorMannheim, Philip D.
dc.date1995-08-09
dc.date.accessioned2026-07-07T02:19:59Z
dc.date.available2026-07-07T02:19:59Z
dc.descriptionWe make a first application of the linear gravitational potentials of the conformal gravity theory to the distance scale associated with clusters of galaxies, with the theory being found to give a reasonable value for the mean velocity of the virialized core of the typical Coma cluster, with no need to invoke the existence of dark matter.
dc.descriptionPlain TeX, 4 pages. To appear in the Proceedings of the 1995 Astronomical Society of the Pacific Symposium on Clusters, Lensing, and the Future of the Universe, University of Maryland, June 1995
dc.identifierhttps://arxiv.org/abs/astro-ph/9508045
dc.identifierhttp://arxiv.org/abs/astro-ph/9508045
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10081
dc.subjectAstrophysics
dc.titleLinear Potentials in the Cores of Clusters of Galaxies
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