Origin of the complex iron line structure and spectral variation in Mrk 766
Abstract
Complex Fe-K emission/absorption line features are commonly observed in the 6-11 keV band from Active Galactic Nuclei (AGN). These features are formed in various physical components surrounding the black holes. The Narrow-Line Seyfert 1 (NLS1) galaxy Mrk 766, in particular, exhibits characteristic blue-shifted Fe-K absorption lines caused by the ultrafast outflow (UFO), and a broad Fe-K emission line, as well as variable absorbers partially covering the X-ray emitting region. We re-analyse the Mrk 766 archival data of XMM-Newton, NuSTAR, and Swift to investigate the origin of the Fe-K line feature and the 0.3-79 keV energy spectral variation. We have found that the spectral variation in ≲10 keV is primarily explained by the variable partial covering of the central X-ray source by multilayer absorbing clouds. The Fe-K line feature consists of the blue-shifted absorption lines due to the UFO, a narrow emission line from the distant material, a broad emission line from the inner-disc reflection, and a slightly broadened weak emission line at around 6.4-6.7 keV whose equivalent width is ~0.05 keV. The last one is presumably due to the resonance scattering in the UFO out of the line-of-sight, as predicted by a Monte Carlo simulation based on the hydrodynamical UFO modelling. We suggest that the seemingly complex Fe-K line features and the X-ray energy spectra of Mrk 766 are explained by a moderately extended central X-ray source around a Schwarzschild black hole, an optically thick accretion disc with a truncated inner-radius, the UFO, multilayer partial covering clouds, and a torus.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- October 2023
- DOI:
- 10.1093/mnras/stad2329
- arXiv:
- arXiv:2308.05924
- Bibcode:
- 2023MNRAS.525..922M
- Keywords:
-
- galaxies: active;
- galaxies: Seyfert;
- X-rays: individual: Mrk 766;
- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 11 pages, 7 figures, Published in MNRAS