Dynamical Modeling of SAURON Galaxies

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dc.creatorCappellari, M.
dc.creatorBosch, R. C. E. van den
dc.creatorVerolme, E. K.
dc.creatorBacon, R.
dc.creatorBureau, M.
dc.creatorCopin, Y.
dc.creatorDavies, R. L.
dc.creatorEmsellem, E.
dc.creatorKrajnovic, D.
dc.creatorKuntschner, H.
dc.creatorMcDermid, R.
dc.creatorMiller, B. W.
dc.creatorPeletier, R. F.
dc.creatorde Zeeuw, P. T.
dc.date2003-02-14
dc.date.accessioned2026-07-07T02:07:35Z
dc.date.available2026-07-07T02:07:35Z
dc.descriptionWe describe our program for the dynamical modeling of early-type galaxies observed with the panoramic integral-field spectrograph SAURON. We are using Schwarzschild's numerical orbit superposition method to reproduce in detail all kinematical and photometric observables, and recover the intrinsic orbital structure of the galaxies. Since catastrophes are the most prominent features in the orbital observables, two-dimensional kinematical coverage is essential to constrain the dynamical models.
dc.description5 pages, 4 figures, LaTeX. Published in 2003, Carnegie Observatories Astrophysics Series, Vol. 1: Coevolution of Black Holes and Galaxies, ed. L. C. Ho (Pasadena: Carnegie Observatories, http://www.ociw.edu/ociw/symposia/series/symposium1/proceedings.html)
dc.identifierhttps://arxiv.org/abs/astro-ph/0302274
dc.identifierhttp://arxiv.org/abs/astro-ph/0302274
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5744
dc.subjectAstrophysics
dc.titleDynamical Modeling of SAURON Galaxies
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