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Self-consistent Modelling of the Milky Way using Gaia data
Published online by Cambridge University Press: 07 March 2018
Abstract
Angle/action based distribution function (DF) models can be optimised based on how well they reproduce observations thus revealing the current matter distribution in the Milky Way. Gaia data combined with data from other surveys, e.g. the RAVE/TGAS sample, and its full selection function will greatly improve their accuracy.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 152 - 155
- Copyright
- Copyright © International Astronomical Union 2018
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