CORDIS Project
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The Gaia-ESO Survey aims to understand galaxy formation and evolution by studying the Milky Way. It utilizes high-quality spectroscopy to analyze the chemical composition and kinematics of stars, providing insights into the structure of our galaxy.
Understanding how galaxies actually form and evolve within our dark matter and dark energy dominated [ɅCDM] universe continues to be an enormous challenge.
State of the art simulations of the aggregation of cold dark matter under its own gravitational influence suggest that galaxies grow from very smooth initial conditions through a sequence of merger and accretion events.
However, theoretical models of galaxy formation, which necessarily involve modelling star formation and stellar evolution, t…
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