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Modeling the FeK line profiles in type i active galactic nuclei with a compton-thick disk wind

Tatum, M M; Turner, T J; Sim, Stuart A; Miller, L; Reeves, J N; Patrick, A R; Long, K S

Description

We have modeled a small sample of Seyfert galaxies that were previously identified as having simple X-ray spectra with little intrinsic absorption. The sources in this sample all contain moderately broad components of FeK-shell emission and are ideal candidates for testing the applicability of a Compton-thick accretion disk wind model to active galactic nucleus (AGN) emission components. Viewing angles through the wind allow the observer to see the absorption signature of the gas, whereas...[Show more]

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
URI: http://hdl.handle.net/1885/67918
Source: Astrophysical Journal, The
DOI: 10.1088/0004-637X/752/2/94

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