Modeling of the broad band X-ray spectra of the Seyfert Mrk 841
Abstract
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.
- Publication:
-
Revista Mexicana de Astronomia y Astrofisica Conference Series
- Pub Date:
- April 2008
- Bibcode:
- 2008RMxAC..32..104P
- Keywords:
-
- galaxies: Seyfert;
- galaxies: individual (Mrk 841);
- X-rays: galaxies