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Galactic dynamics and radial migration

Published online by Cambridge University Press:  17 July 2015

R. Schönrich
R. Schönrich*
Affiliation:
Rudolf-Peierls-Centre for Theoretical physics, 1 Keble Road, Oxford OX1 3NP, UK
*
e-mail: ralph.schoenrich@physics.ox.ac.uk
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Abstract

In this proceeding I will shortly discuss radial migration in disc galaxies and the Milky Way in particular. I discuss the most important evidence for radial migration, i.e. the increasing width of the metallicity distribution with age, while the mean metallicity of stars remains constant. In the second part I briefly discuss thick disc creation by migration, the question of preferential migration with vertical action and its impact on Galactic kinematics.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 68: The Milky Way Unravelled by Gaia: GREAT Science from the Gaia Data Releases , 2014 , pp. 339 - 345
Copyright
© EAS, EDP Sciences, 2015

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