Kinematics of the disk population in the GAIA era

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dc.creatorBertelli, G.
dc.creatorVallenari, A.
dc.creatorPasetto, S.
dc.creatorChiosi, C.
dc.date2002-12-05
dc.date.accessioned2026-07-07T02:06:43Z
dc.date.available2026-07-07T02:06:43Z
dc.descriptionGAIA data will create a precise 3-dimensional map of the Galaxy, providing positional information, radial velocities, luminosity, temperature and chemical composition of a representative sample of stars. Here we present a new implementation of the Padova Galaxy Model, where kinematics simulations are included. A few examples of application to GAIA science are discussed, in particular concerning radial velocities determinations of the thin and thick disk.
dc.description6 pages, 3 figures, Proceedings of the conference:"Gaia Spectroscopy: Science and Technology"
dc.identifierhttps://arxiv.org/abs/astro-ph/0212136
dc.identifierhttp://arxiv.org/abs/astro-ph/0212136
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5460
dc.subjectAstrophysics
dc.titleKinematics of the disk population in the GAIA era
dc.typetext

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