Triaxial analytical potential-density pairs for galaxies

dc.creatorVogt, D
dc.creatorLetelier, PS
dc.date2007
dc.date2014-08-01T18:20:00Z
dc.date2015-11-26T18:02:49Z
dc.date2014-08-01T18:20:00Z
dc.date2015-11-26T18:02:49Z
dc.date.accessioned2018-03-29T00:44:33Z
dc.date.available2018-03-29T00:44:33Z
dc.identifierPublications Of The Astronomical Society Of Japan. Astronomical Soc Japan, v. 59, n. 2, n. 319, n. 322, 2007.
dc.identifier0004-6264
dc.identifierWOS:000246404000005
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/77393
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/77393
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1292346
dc.descriptionWe present two triaxial analytical potential-density pairs that can be viewed as generalized versions of the axisymmetric Miyamoto-Nagai and Satoh galactic models. These potential-density pairs may be useful models for galaxies with box-shaped bulges. The resulting mass-density distributions are everywhere non-negative and free from singularities. Also, a few numerically calculated orbits for the Miyamoto-Nagai-like triaxial potential are presented.
dc.description59
dc.description2
dc.description319
dc.description322
dc.languageen
dc.publisherAstronomical Soc Japan
dc.publisherTokyo
dc.publisherJapão
dc.relationPublications Of The Astronomical Society Of Japan
dc.relationPubl. Astron. Soc. Jpn.
dc.rightsfechado
dc.sourceWeb of Science
dc.subjectgalaxies : structure
dc.subjectgalaxies : kinematics and dynamics
dc.subjectPeanut-shaped Bulges
dc.subjectSpherical Galaxies
dc.subjectModels
dc.subjectDisks
dc.titleTriaxial analytical potential-density pairs for galaxies
dc.typeArtículos de revistas


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