Revisiting the (V/sigma)-epsilon anisotropy diagram of early-type galaxies using integral-field kinematics

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dc.creatorCappellari, M.
dc.creatorBacon, R.
dc.creatorBureau, M.
dc.creatorDavies, R. L.
dc.creatorde Zeeuw, P. T.
dc.creatorEmsellem, E.
dc.creatorFalcon-Barroso, J.
dc.creatorKrajnovic, D.
dc.creatorKuntschner, H.
dc.creatorMcDermid, R. M.
dc.creatorPeletier, R. F.
dc.creatorSarzi, M.
dc.creatorBosch, R. C. E. van den
dc.creatorvan de Ven, G.
dc.date2005-09-15
dc.date.accessioned2026-07-07T02:18:40Z
dc.date.available2026-07-07T02:18:40Z
dc.descriptionWe use integral-field observation of the stellar kinematics obtained with SAURON in combination with Schwarzschild dynamical models to revisit our understanding of the classic (V/sigma)-epsilon anisotropy diagram of early-type galaxies.
dc.description4 pages, 3 figures, LaTeX. To appear on the web proceedings of "Nearly Normal Galaxies in a LCDM Universe. A conference celebrating the 60th birthdays of George Blumenthal, Sandra Faber and Joel Primack". Santa Cruz, CA, 2005 (see http://astro.ucsc.edu/~nng/)
dc.identifierhttps://arxiv.org/abs/astro-ph/0509470
dc.identifierhttp://arxiv.org/abs/astro-ph/0509470
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9578
dc.subjectAstrophysics
dc.titleRevisiting the (V/sigma)-epsilon anisotropy diagram of early-type galaxies using integral-field kinematics
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