Multidimensional modelling of X-ray spectra for AGN accretion disc outflows

S.A. Sim, K.S. Long, L. Miller, T.J. Turner

Research output: Contribution to journalArticlepeer-review

68 Citations (Scopus)

Abstract

We use a multidimensional Monte Carlo code to compute X-ray spectra for a variety of active galactic nucleus (AGN) disc-wind outflow geometries. We focus on the formation of blueshifted absorption features in the Fe K band and show that line features similar to those which have been reported in observations are often produced for lines of sight through disc-wind geometries. We also discuss the formation of other spectral features in highly ionized outflows. In particular, we show that, for sufficiently high wind densities, moderately strong Fe K emission lines can form and that electron scattering in the flow may cause these lines to develop extended red wings. We illustrate the potential relevance of such models to the interpretation of real X-ray data by comparison with observations of a well-known AGN, Mrk 766. Journal compilation
Original languageEnglish
Pages (from-to)611-624
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume388
Issue number2
DOIs
Publication statusPublished - 01 Aug 2008

Bibliographical note

Copyright 2011 Elsevier B.V., All rights reserved.

Fingerprint Dive into the research topics of 'Multidimensional modelling of X-ray spectra for AGN accretion disc outflows'. Together they form a unique fingerprint.

Cite this