X-Ray Properties of a High-Redshift Cluster

Details X-Ray Properties of a High-Redshift Cluster X-Ray Properties of a High-Redshift Cluster

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..322g&link_type=abstract

Chandra Proposal ID #01800048

Physics

Chandra Proposal Id #01800048

Scientific paper

The mass of X-ray emitting gas in rich clusters can considerably exceed the mass in stars, and is enriched in heavy elements. The origin and evolution of this intracluster medium are not fully understood. This observation of an X-ray-bright cluster at z = 0.83 will give insight into the mass, temperature and metal distribution of the medium at an early epoch, as well as measurement of the gravitational potential.

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