Tracking Fe K-shell emission from the Accretion Disk of Mkn 205

Details Tracking Fe K-shell emission from the Accretion Disk of Mkn 205 Tracking Fe K-shell emission from the Accretion Disk of Mkn 205

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...50g&link_type=abstract

XMM-Newton Proposal ID #04012401

Computer Science

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Mkn 205, Xmm-Newton Proposal 04012401

Scientific paper

XMM and Chandra data have recently revealed complex and exciting behavior in the Fe K-band of Seyfert-type AGN. These include rapid variations in line energy, characteristic of gas orbiting a central black hole, and a tight correlation of the ionized line component with flux. These strengthen the assertion a significant fraction of Fe Ka emission is from the accretion disk. We have searched the XMM archive for AGN where line emission appears dominated by the inner disk. Mkn 205 is the best target for continuing Fe Ka studies in XMM cycle 5, and we propose a 120 ks observation of this quasar.

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