
TY  - JOUR
A1  - Reylé, Céline 
A1  - Robin, Annie C. 
A1  - Picaud, Sébastien 
T1  - Kinematics of the Galactic Bulge from Radial Velocity and Proper Motion Optical Surveys
JF  - Publications of the Astronomical Society of Australia
JO  - Publ. Astron. Soc.  Aust.
Y1  - 2004
VL  - 21
IS  - 2
SP  - 138
EP  - 143
KW  - Galaxy: bulge &#8212; Galaxy: kinematics and dynamics &#8212; surveys
UR  - https://doi.org/10.1071/AS04016 
N2  - Large-scale surveys provide new constraints on the structure and evolution of the Milky Way. The population synthesis approach is a useful tool to interpret such data sets and to test scenarios of evolution of the Galaxy. New constraints on Galactic parameters have been obtained from the Besan&#231;on model of population synthesis, in particular in the inner regions, thanks to near-infrared surveys less affected by interstellar extinction than the optical ones. We present here a few preliminary comparisons between observed and simulated distributions of proper motions in the direction of the Galactic bulge. Next we discuss how bulge stars can be observed and separated from other populations with the RAVE and Gaia surveys. 
ER  -

