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Multi-dimensional modelling of X-ray spectra for AGN accretion-disk outflows

Abstract:

We use a multi-dimensional Monte Carlo code to compute X-ray spectra for a variety of active galactic nucleus (AGN) disk-wind outflow geometries. We focus on the formation of blue-shifted 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 disk-wind geometries. We also discuss the formation of other spectral features in highly ionized outflows. In particular we show that, for s...

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Publication status:
Published

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Turner, TJ More by this author
Journal:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume:
388
Issue:
2
Pages:
611-624
Publication date:
2008-05-15
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:50270ad2-d450-4406-8276-73cb0041393c
Source identifiers:
14603
Local pid:
pubs:14603
Language:
English
Keywords:

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