X-ray clues on the ultimate fate of compact radio sources

Details X-ray clues on the ultimate fate of compact radio sources X-ray clues on the ultimate fate of compact radio sources

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..255g&link_type=abstract

XMM-Newton Proposal ID #04070308

Other

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, 4C+00.02, Pks0428+20, 4C+14.41, Pks1607+26, Pks2008-608, 2210+016, Xmm-Newton Proposal 04070308

Scientific paper

Are compact radio galaxies intrinsically X-ray weak? Do they otherwise live in dense environments? If the latter is true, does the nuclear gas affect the jet evolution in radio-loud Active Galactic Nuclei (AGN)? In order to answer these questions, we propose to observe within the XMM-Newton AO5 a radio-selected complete sample of Giga-Hertz Peaked (GPS) galaxies. We request 9 objects, for a total allocation time of 210 ks. The proposed observations will provide clues on the nature of compact radio sources, and on the ultimate fate of small-scale radio structure evolution.

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