Orbital structure of triaxial galaxies

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dc.creatorvan de Ven, Glenn
dc.creatorVerolme, Ellen
dc.creatorCappellari, Michele
dc.creatorde Zeeuw, Tim
dc.date2003-10-17
dc.date.accessioned2026-07-07T02:10:34Z
dc.date.available2026-07-07T02:10:34Z
dc.descriptionWe have developed a method to construct realistic triaxial dynamical models for elliptical galaxies, allowing us to derive best-fitting parameters, such as the mass-to-light ratio and the black hole mass, and to study the orbital structure. We use triaxial theoretical Abel models to investigate the robustness of the method.
dc.description2 pages (1 figure), to appear in the proceedings of the IAU Symposium 220 "Dark matter in galaxies", eds. S. Ryder, D.J. Pisano, M. Walker and K. Freeman
dc.identifierhttps://arxiv.org/abs/astro-ph/0310488
dc.identifierhttp://arxiv.org/abs/astro-ph/0310488
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6778
dc.subjectAstrophysics
dc.titleOrbital structure of triaxial galaxies
dc.typetext

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