X-ray Environment of Radio Galaxy 4C 29.30

Details X-ray Environment of Radio Galaxy 4C 29.30 X-ray Environment of Radio Galaxy 4C 29.30

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..156s&link_type=abstract

XMM-Newton Proposal ID #05041201

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, 4C 29.30, Xmm-Newton Proposal 05041201

Scientific paper

We propose to observe a radio galaxy, 4C 29.30 with XMM-Newton for 40ksec in order to study (1) the spectral properties of the nucleus; and (2) search for X-ray emission associated with the radio halo surrounding this source. This low redshift galaxy is embedded in a rich environment studied in optical and radio bands. The radio jets end just outside the host galaxy and this 60kpc structure is embedded in a ~600kpc radio halo. The good quality X-ray observations are missing. A short ~8ksec Chandra archival data with a low S/N do not allow for detailed analysis. Our new XMM-Newton observation will provide the best quality X-ray spectra of the radio core. The large field of view of the XMM-Newton is required for studies of any large scale emission associated with the radio halo.

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