Cool Molecular Gas in Cooling Flow Clusters

Details Cool Molecular Gas in Cooling Flow Clusters Cool Molecular Gas in Cooling Flow Clusters

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop.3161j&link_type=abstract

Spitzer Proposal ID #3161

Physics

Scientific paper

As part of a large ongoing multiwavelength study into the nature and energetics of the cool and cold phases of the intra cluster medium of clusters of galaxies, we propose to search for rotational H_2 lines from 100-200 Kelvin gas at the centres of these clusters. The cool gas has several possible origins, including having cooled from the hot phase of the intra cluster medium. In any event, a full understanding of its nature is key to our understanding of galaxy formation and evolution.

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