Modeling of the broad band X-ray spectra of the Seyfert Mrk 841

Details Modeling of the broad band X-ray spectra of the Seyfert Mrk 841 Modeling of the broad band X-ray spectra of the Seyfert Mrk 841

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..32..104p&link_type=abstract

The Nuclear Region, Host Galaxy and Environment of Active Galaxies (Eds. Erika Benítez, Irene Cruz-González, & Yair Krongold) Re

Astronomy and Astrophysics

Astronomy

Galaxies: Seyfert, Galaxies: Individual (Mrk 841), X-Rays: Galaxies

Scientific paper

The presence in Mrk 841 of a strong soft excess and a complex iron profile, has been confirmed by repeated XMM-Newton observations. The 0.5-10 keV emission may be entirely explained by the combination of a relativistically blurred photoionized reflection, producing simultaneously the soft excess and the broad iron line, and a neutral, unblurred one, producing the narrow line.

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