Star formation history and dynamical evolution of the solar neighbourhood
Abstract
We used our detailed analytic local disc model to compare predictions in number counts, colour distribuitons and kinematics with a data set extracted from a combination of TGAS and RAVE catalogues. We find generally a very good agreement with some deviations close to the Galactic plane.
- Publication:
-
Rediscovering Our Galaxy
- Pub Date:
- August 2018
- DOI:
- Bibcode:
- 2018IAUS..334..310J
- Keywords:
-
- Galaxy: disk;
- Galaxy: kinematics and dynamics;
- Galaxy: evolution;
- Galaxy: solar neighbourhood