Illuminating the evolution of CNOC2 group galaxies with MIPS at 24microns

Details Illuminating the evolution of CNOC2 group galaxies with MIPS at 24microns Illuminating the evolution of CNOC2 group galaxies with MIPS at 24microns

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop30827r&link_type=abstract

Spitzer Proposal ID #30827

Computer Science

Scientific paper

Groups of galaxies play a critical role in the global evolution of galaxies, as their dynamics make them the ideal environment to foster galaxy-galaxy interactions and mergers, generating infrared-bright dusty starbursts and leading to a dramatic transformation of the galaxy properties. As groups today contain ~60% of the galaxy population, and are the first super-galactic step in the hierarchical growth tree which dominates structure formation, these environments must have a critical influence on the evolution of star formation in the Universe as a whole. To study the evolution of star formation in groups requires highly complete, targetted, deep spectroscopic surveys; the only such survey is our sample of 26 groups at 0.3

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