Kinematics of the disk population in the GAIA era
Astrophysics
2007-05-23 v1
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.
Cite
@article{arxiv.astro-ph/0212136,
title = {Kinematics of the disk population in the GAIA era},
author = {G. Bertelli and A. Vallenari and S. Pasetto and C. Chiosi},
journal= {arXiv preprint arXiv:astro-ph/0212136},
year = {2007}
}
Comments
6 pages, 3 figures, Proceedings of the conference:"Gaia Spectroscopy: Science and Technology"