Physics
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...47b&link_type=abstract
XMM-Newton Proposal ID #02009102
Physics
3C 109, 4C+74.26, Xmm-Newton Proposal 02009102
Scientific paper
We propose to observe two high luminosity broad-line radio galaxies (BLRGs): 3C109 (z0.31), the most X-ray luminous BLRG known and the most X-ray luminous object in which a broad iron line was detected with ASCA, and 4C+74.26 (z0.10), a young, bright BLRG which also had a broad Fe K ASCA detection. A 40 ks observation of 3C109 and a 35 ks observation of 4C+74.26 with XMM-Newton will allow the first precise determination of the Fe K line properties in luminous radio-loud active galaxies. The resulting constraints on the disc inclination angle and inner radius will be of great significance for the understanding of jet formation and accretion physics in luminous radio galaxies.
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