Do hybrid morphology radio sources form in a lopsided distribution of cold gas?

Details Do hybrid morphology radio sources form in a lopsided distribution of cold gas? Do hybrid morphology radio sources form in a lopsided distribution of cold gas?

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..199m&link_type=abstract

XMM-Newton Proposal ID #06747402

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, B2 1404+25A, B2 1345+28

Scientific paper

We test the hypothesis that hybrid morphology radio sources (HYMORS; Gopal-Krishna & Wiita 2000) feature one-sided jet disruption caused by propagation into a large-scale overdensity of cold gas, through XMM-Newton observations of B2 1404+25A and B2 1345+28 (33 and 16 ks, respectively). These HYMORS are intrinsic low-inclination RLQs for which the X-ray spectra would ordinarily be unabsorbed. VLBA mapping places the FRI jet on the near side in B2 1404+25A, and so the putative disrupting medium can be directly detected as absorption against the core; in contrast, the FRII lobe is closer in B2 1345+28, and so a simple power-law X-ray spectrum is anticipated. Distinct results are predicted for alternative scenarios of HYMORS formation.

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