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MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND

Abstract:

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 fac...

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Publication status:
Published

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Publisher copy:
10.1088/0004-637X/752/2/94

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Publisher:
Institute of Physics Publishing
Journal:
ASTROPHYSICAL JOURNAL More from this journal
Volume:
752
Issue:
2
Pages:
94-94
Publication date:
2012-06-20
DOI:
EISSN:
1538-4357
ISSN:
0004-637X
Language:
English
Keywords:
Pubs id:
pubs:342647
UUID:
uuid:f7fe8442-a54d-4685-9f0d-ab540b186298
Local pid:
pubs:342647
Source identifiers:
342647
Deposit date:
2012-12-19

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