Exact density-potential pairs from the holomorphic Coulomb field

Simple item page
dc.creatorCiotti, L.
dc.creatorGiampieri, G.
dc.date2007-01-12
dc.date.accessioned2026-07-07T10:21:29Z
dc.date.available2026-07-07T10:21:29Z
dc.descriptionWe show how the complex-shift method introduced by Appell in gravity to the case of a point mass (and applied among others in electrodynamics by Newman, Carter, Lynden-Bell, and Kaiser to determine remarkable properties of the electromagnetic field of rotating charged configurations), can be extended to obtain new and explicit density-potential pairs for self-gravitating systems departing significantly from spherical symmetry. The rotational properties of two axysimmetric baroclinic gaseous configurations derived with the proposed method are illustrated.
dc.description8 pages, 2 figures, MNRAS accepted
dc.identifierhttps://arxiv.org/abs/astro-ph/0701388
dc.identifierhttp://arxiv.org/abs/astro-ph/0701388
dc.identifierMon.Not.Roy.Astron.Soc.376:1162-1168,2007
dc.identifierdoi:10.1111/j.1365-2966.2007.11497.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175188
dc.subjectAstrophysics
dc.titleExact density-potential pairs from the holomorphic Coulomb field
dc.typetext

Files

Collections

arXiv