The Coordinated Growth of Stars, Haloes and Large-Scale Structure Since z=1

Details The Coordinated Growth of Stars, Haloes and Large-Scale Structure Since z=1 The Coordinated Growth of Stars, Haloes and Large-Scale Structure Since z=1

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..379..109b&link_type=abstract

Cosmic Frontiers ASP Conference Series, Vol. 379, proceedings of the conference held 31 July-4 August 2006 at Durham University,

Physics

Scientific paper

In this review I summarize recent observational efforts to determine how the evolution of galaxy colours and star formation rates depends on their stellar mass and their environment. These observations are compared with the latest theoretical models. Although a consistent picture of galaxy formation is beginning to emerge, in which energetic feedback mechanisms play an important role, some interesting puzzles remain, especially regarding the physical processes at work in dense environments.

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