Reduced Cooling & Feedback in Cluster Cooling Flows

Details Reduced Cooling & Feedback in Cluster Cooling Flows Reduced Cooling & Feedback in Cluster Cooling Flows

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1315m&link_type=abstract

Chandra Proposal ID #04800521

Computer Science

Chandra Proposal Id #04800521

Scientific paper

We propose to observe three galaxy clusters to examine the effects of energy feedback into the cooling intracluster medium from supernovae, radio sources, and cluster mergers. The observations are designed to test cooling flow models by comparing the X-ray cooling rates to star formation rates on fine spatial scales. The observations will test the universality of emerging correlations between strong nebular emission, sites of massive star formation, and bright X-ray structures in central cluster galaxies, where enhanced cooling may be occurring. The data will allow us to evaluate the likelihood that the large star formation rates and Balmer emission in the central galaxies are related or unrelated to cooling flows.

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