A Closer Look at 4C+74.26 with XMM-Newton: Focusing on the Disk-Jet Interaction

Details A Closer Look at 4C+74.26 with XMM-Newton: Focusing on the Disk-Jet Interaction A Closer Look at 4C+74.26 with XMM-Newton: Focusing on the Disk-Jet Interaction

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..121b&link_type=abstract

XMM-Newton Proposal ID #04030601

Other

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, 4C+74.26, Xmm-Newton Proposal 04030601

Scientific paper

We propose a 70 ks follow-up observation of the bright broad-line radio galaxy 4C+74.26. A previous 35 ks XMM-Newton observation of 4C+74.26 yielded the first indication of a relativistically broadened Fe Kalpha line in a radio-loud AGN as well as other typical AGN properties (e.g., a warm absorber). Doubling the observing time, as proposed here, will allow a detailed investigation of the Fe Kalpha line profile, and hence the first accurate determination of the geometry and structure of the inner accretion disk in a radio-loud AGN. This information will be invaluable for modeling the physics of the disk-jet interaction.

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