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Kinematics of the disk population in the GAIA era

G. Bertelli·A. Vallenari·S. Pasetto·C. Chiosi
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Abstract

GAIA 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.

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G. Bertelli, A. Vallenari, S. Pasetto, C. Chiosi. 2002-12-05. Kinematics of the disk population in the GAIA era. https://arxiv.org/abs/astro-ph/0212136

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