Spectroscopic surveys to measure Galaxy evolution

Details Spectroscopic surveys to measure Galaxy evolution Spectroscopic surveys to measure Galaxy evolution

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..265..470g&link_type=abstract

Chemical Abundances in the Universe: Connecting First Stars to Planets, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

Surveys, Stellar Spectroscopy, Gaia, Galaxy Evolution

Scientific paper

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.

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