Modeling the Milky Way disk dynamics
Modeling the Milky Way disk dynamics
Modeling the Milky Way disk dynamics
- No tags were found...
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
Beyond <strong>the</strong> solar neighbourhoodAntoja et al. 2012•First detection ofnon-local disckinematic substructureR~8.4 kpcR~7.8 kpcR~7.2 kpc•Local known groupsare still observed at 1kpc in <strong>the</strong> solar circle•Known groups areshifted in velocityinside and outside solarcircle•More changes inradius than in azimuthT. Antoja Sydney, 24/07/2012