Detection of High Redshift Cluster of Galaxies around 3CR184

Details Detection of High Redshift Cluster of Galaxies around 3CR184 Detection of High Redshift Cluster of Galaxies around 3CR184

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop.1002m&link_type=abstract

Chandra Proposal ID #03800590

Computer Science

Chandra Proposal Id #03800590

Scientific paper

This proposal is to separate the cluster gas and AGN components in the high redshift cluster of galaxies of 3CR184. ASCA observation of 3CR184 has suggested the existence of the large cluster of galaxies and/or AGN. The good spatial resolution of Chandra is the only way to separate the two components, and to prove the existence of a large cluster of galaxies at z=1. The flux and metal abundance of high redshift clusters of galaxies are particularly important to understand the evolution of clusters and the structure formation in the universe.

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