The dynamics of low-power (FRI) jets

Details The dynamics of low-power (FRI) jets The dynamics of low-power (FRI) jets

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop...54c&link_type=abstract

XMM-Newton Proposal ID #05517201

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, 3C 31, Xmm-Newton Proposal Id #05517201

Scientific paper

The dynamics of low-power radio jets are largely determined by interactions with the surrounding X-ray emitting gas. With previous XMM-Newton observations, we have detected evidence for radio-source heating and have used environmental measurements to constrain detailed three-dimensional kinematic models of jet dynamics. Here we propose to reobserve one of the best candidates for this type of study, 3C 31, for which our previous observation was unusable due to flare contamination, and to observe for the first time the lower luminosity radio galaxy B2 1553+24, in order to determine the physical properties of the jets and to investigate their interactions with the environment.

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