High-Redshift Clusters and Classical Doubles with Cigar-Shaped Radio Bridges

Details High-Redshift Clusters and Classical Doubles with Cigar-Shaped Radio Bridges High-Redshift Clusters and Classical Doubles with Cigar-Shaped Radio Bridges

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..688d&link_type=abstract

Chandra Proposal ID #02800376

Physics

Chandra Proposal Id #02800376

Scientific paper

We propose (1) to study the properties of the intracluster medium (ICM) in high- redshift clusters of galaxies; (2) to determine the accuracy with which ambient gas densities can be estimated using the radio properties of FRIIb radio sources; and (3) to study the X-ray properties of the radio cores, hotspots, and lobes/ bridges of FRIIb radio sources. We propose to observe 4 unambiguously-extended X-ray sources for which we have estimated ambient gas densities from radio observations. The targets, 3C254, 3C275.1, 3C280, and 3C220 are extremely radio loud FRII radio sources with regular radio bridges. Their properties span z=0.6-1.0, radio galaxies to quasars, and radio sizes 165-265 kpc.

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