Kinematics of the Galactic populations in the GAIA era

被引：0
|
作者：
Bertelli, G [1 ]
Vallenari, A [1 ]
Pasetto, S [1 ]
Chiosi, C [1 ]
机构：
[1] Osserv Astron Padova, INAF, I-35122 Padua, Italy
来源：
GAIA SPECTROSCOPY, SCIENCE AND TECHNOLOGY, PROCEEDINGS | 2003年 / 298卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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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页码：153 / 158
页数：6
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