MCG--2-58-22: a truncated yet ionized accretion disk?

Details MCG--2-58-22: a truncated yet ionized accretion disk? MCG--2-58-22: a truncated yet ionized accretion disk?

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop...72m&link_type=abstract

XMM-Newton Proposal ID #06027801

Computer Science

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Mcg-2-58-22

Scientific paper

We propose a 106 ks observation XMM-Newton long-look to study the Fe K emission complex of the Seyfert 1.5 AGN MCG-2-58-22, which has the unique combination of being X-ray bright, ``bare'' (i.e., lacking a strong ionized absorber), and possibly hosting both a truncated accretion disk and ionized circumnuclear material. We aim to accurately constrain the geometry and ionization state of the accreting circumnuclear material of this low-Compton reflection source by resolving the Fe Kalpha line and constraining its origin, which may likely be a truncated thin disk, and verifying a previous claim of emission from H-like Fe. We will also determine the origin of this object's soft excess.

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