XMM-Newton Proposal 02018603

Details XMM-Newton Proposal 02018603 XMM-Newton Proposal 02018603

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..100c&link_type=abstract

XMM-Newton Proposal ID #02018603

Physics

3C 296, 3C 76.1, Ngc 1044, Xmm-Newton Proposal 02018603

Scientific paper

The structure of low-power radio galaxies is thought to be determined largely by interactions with the group atmosphere in which these objects typically reside. Detailed observations of these atmospheres can answer long-standing questions about physical conditions in radio galaxies, their dynamics and evolution. Our XMM GO observations of two such objects provide strong evidence for the influence of environment on radio-lobe structure, illustrating that XMM's high sensitivity to large-scale X-ray emission is ideally suited to this work. We propose to continue this observational programme by observing three more well-studied twin-jet sources, enlarging our sample to include examples of all typical FR-I radio-lobe morphologies.

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