3-Dimensional Kinematics in low foreground extinction windows of the   Galactic Bulge: Radial Velocities for 6 bulge fields
  The detailed structure of the Galactic bulge still remain uncertain. The strong difficulties of obtaining observations of stars in the Galactic bulge have hindered the acquisition of a kinematic representation for the inner kpc of the Milky Way. The observation of the 3-d kinematics in several low foreground extinction windows can solve this problem. We have developed a new technique, which combines precise stellar HST positions and proper motions with integral field spectroscopy, in order to obtain reliable 3-d stellar kinematics in crowded fields of the Galactic center. In addition, we present results using the new techniques for six fields in our project. A significant vertex deviation has been found in some of the fields in agreement with previous determinations. This result confirms the presence of a stellar bar in the Galactic bulge. 
M. Soto (Leiden Observatory - U. de La Serena), K. Kuijken (Leiden   Observatory), R.M. Rich (UCLA)
astro-ph.GA