Axisymmetric models for galaxies by equipotential and equidensity methods

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dc.creatorJiang, Zhenglu
dc.creatorFang, Daoyuan
dc.creatorMoss, David
dc.date2008-06-08
dc.date.accessioned2026-07-07T09:43:17Z
dc.date.available2026-07-07T09:43:17Z
dc.descriptionIn this paper we outline equipotential and equidensity methods of constructing axisymmetric models for galaxies. The former method defines equipotentials, from which the corresponding densities of the galaxy models can be obtained using Poisson's equation; the latter defines the equidensity surfaces of the galaxy models directly.
dc.identifierhttps://arxiv.org/abs/0806.1304
dc.identifierhttp://arxiv.org/abs/0806.1304
dc.identifierin Li D., Zhang X., Yuan Y., eds., Proceedings of the Sixth Conference of China Society, Industry and Applied Mathematics, Research Information Ltd., Hertfordshire, p. 79-83, 2002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/162501
dc.subjectAstrophysics
dc.titleAxisymmetric models for galaxies by equipotential and equidensity methods
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