Triaxial Orbit-based Models Of Elliptical Galaxies

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dc.creatorBosch, Remco van den
dc.creatorvan de Ven, Glenn
dc.creatorVerolme, Ellen
dc.creatorCappellari, Michele
dc.creatorde Zeeuw, Tim
dc.date2005-12-02
dc.date.accessioned2026-07-07T06:48:59Z
dc.date.available2026-07-07T06:48:59Z
dc.descriptionWe have developed an orbit-based method for constructing triaxial models of elliptical galaxies, which fit their observed surface brightness and kinematics. We have tested the method against analytical models with general distribution functions. Here, we present models that fit integral-field SAURON observations of NGC3379 and NGC4365.
dc.description2 pages (2 figures), Proceedings for the fifth Marseille International Cosmology Conference: "The Fabulous Destiny of Galaxies: Bridging Past and Present", 2005 June 20-24, Marseille
dc.identifierhttps://arxiv.org/abs/astro-ph/0512062
dc.identifierhttp://arxiv.org/abs/astro-ph/0512062
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/104174
dc.subjectAstrophysics
dc.titleTriaxial Orbit-based Models Of Elliptical Galaxies
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