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Star formation history and dynamical evolution of the solar neighbourhood
Published online by Cambridge University Press: 02 August 2018
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 310 - 311
- Copyright
- Copyright © International Astronomical Union 2018