Chemodynamical modelling of the Milky Way

Abstract

Chemodynamical models of our Galaxy that have analytic Extended Distribution Functions (EDFs) are likely to play a key role in extracting science from surveys in the era of Gaia.

6 pages to appear in "Reconstructing the Milky Way history: spectroscopic surveys, asteroseismology and chemodynamical models", eds C Chiappini, J Montalban & M Steffen

References in corpus (7)

• The Radial Velocity Experiment (RAVE): first data release
• Constraining the Galaxy's dark halo with RAVE stars
• Extended distribution functions for our Galaxy
• Action-based distribution functions for spheroidal galaxy components
• The distribution function of the Galaxy's dark halo
• Bringing the Galaxy's dark halo to life
• A fast algorithm for estimating actions in triaxial potentials

Cited by in corpus (3)

• Galactic Archaeology with asteroseismology and spectroscopy: Red giants observed by CoRoT and APOGEE
• The Atari Disk, a Metal-Poor Stellar Population in the Disk System of the Milky Way
• Orbital Torus Imaging: Using Element Abundances to Map Orbits and Mass in the Milky Way