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Spectroscopic surveys to measure Galaxy evolution

Published online by Cambridge University Press:  09 March 2010

Gerard Gilmore
Gerard Gilmore*
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK email: gil@ast.cam.ac.uk
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Abstract

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Galaxies are complex non-linear systems, evolving on all time-scales. Isolating whatever set of physical processes was important at each major phase of their evolution requires artefacts which resolve the timescales of dominant physical processes. These are the chemical elements, and stellar kinematics. I consider what surveys are required to make progress in Galaxy evolution mapping, in the era of Gaia.

Keywords

Surveysstellar spectroscopyGaiagalaxy evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S265: Chemical Abundances in the Universe: Connecting First Stars to Planets , August 2009 , pp. 470 - 475
Copyright
Copyright © International Astronomical Union 2010

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