Triaxial Halos and Cusps

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dc.creatorSigurdsson, Steinn
dc.creatorMihos, Chris
dc.creatorHernquist, Lars
dc.creatorNorman, Colin
dc.date1998-05-29
dc.date.accessioned2026-07-07T02:27:04Z
dc.date.available2026-07-07T02:27:04Z
dc.descriptionWe present $N$--body models for triaxial elliptical galaxies or halos of galaxies, which are fully self--gravitating, have near constant axis ratio as a function of radius and a $r^{-1}$ central density cusp. Preliminary investigation suggests the model are stable and orbit analysis shows no indication of chaotic orbits. The models provide a starting point for investigations into the evolution of triaxial figures of equilibrium, response of triaxial figures to central black holes, external perturbations and interactions.
dc.description3 pages paspconf latex, includes 2 postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9805369
dc.identifierhttp://arxiv.org/abs/astro-ph/9805369
dc.identifierPubl.Astron.Soc.Pac. 136 (1998) 388-390
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12537
dc.subjectAstrophysics
dc.titleTriaxial Halos and Cusps
dc.typetext

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