English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Tools annual

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

The detailed structure of the Galactic bulge still remain uncertain. Thestrong difficulties of obtaining observations of stars in the Galactic bulgehave hindered the acquisition of a kinematic representation for the inner kpcof the Milky Way. The observation of the 3-d kinematics in several lowforeground extinction windows can solve this problem. We have developed a newtechnique, which combines precise stellar HST positions and proper motions withintegral field spectroscopy, in order to obtain reliable 3-d stellar kinematicsin crowded fields of the Galactic center. In addition, we present results usingthe new techniques for six fields in our project. A significant vertexdeviation has been found in some of the fields in agreement with previousdeterminations. This result confirms the presence of a stellar bar in theGalactic bulge.

3-Dimensional Kinematics in low foreground extinction windows of the Galactic Bulge: Radial Velocities for 6 bulge fields