XMM-Newton Proposal 02032802

Details XMM-Newton Proposal 02032802 XMM-Newton Proposal 02032802

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..174h&link_type=abstract

XMM-Newton Proposal ID #02032802

Physics

3C33, 3C192, Xmm-Newton Proposal 02032802

Scientific paper

Although a good deal of indirect evidence points towards moderate or poor groups as the environment of low-luminosity (and therefore typical) FRII radio galaxies, there are almost no direct X-ray observations of the required hot, confining medium. An FRII radio source would have a dramatic effect on the gas in a group, heating and potentially expelling a significant fraction of it, with important consequences for our understanding of group evolution. In order to characterize the X-ray environments of typical FRII sources, we propose a small survey of the nearest few FRII sources of intermediate size drawn from the well-studied 3CRR catalogue. Our observations will allow us to detect, and measure the properties of, group-scale emission around our targets.

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