XMM-Newton Proposal 03052902

Details XMM-Newton Proposal 03052902 XMM-Newton Proposal 03052902

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..167c&link_type=abstract

XMM-Newton Proposal ID #03052902

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, 3C 31, Ngc 315, Xmm-Newton Proposal 03052902

Scientific paper

The dynamics of low-power radio jets are largely determined by interactions with the surrounding X-ray emitting gas. Our previous Chandra and XMM-Newton observations of radio-galaxy environments have demonstrated the importance of X-ray observations in constraining the physical conditions and dynamics of radio galaxies on small and large scales. Here we propose to observe two of the best-studied FRI radio galaxies, for which we have high-resolution radio data and three-dimensional kinematic models, with the aim of measuring density and pressure in the X-ray emitting environment so as to constrain the jet models, to allow physical properties of the jets to be determined, and to investigate large-scale jet/environment interactions.

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