THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9

We present an analysis of all XMM-Newton and Suzaku X-ray spectra of the nearby luminous Seyfert galaxy Fairall 9. Confirming previous analyses, we find robust evidence for a broad iron line associated with X-ray reflection from the innermost accretion disk. By fitting a spectral model that includes...

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Main Authors: Lohfink, Anne M., Reynolds, Christopher S., Miller, Jon M., Brenneman, Laura W., Mushotzky, Richard F., Nowak, Michael A., Fabian, Andrew C.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/95500
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author Lohfink, Anne M.
Reynolds, Christopher S.
Miller, Jon M.
Brenneman, Laura W.
Mushotzky, Richard F.
Nowak, Michael A.
Fabian, Andrew C.
author2 MIT Kavli Institute for Astrophysics and Space Research
author_facet MIT Kavli Institute for Astrophysics and Space Research
Lohfink, Anne M.
Reynolds, Christopher S.
Miller, Jon M.
Brenneman, Laura W.
Mushotzky, Richard F.
Nowak, Michael A.
Fabian, Andrew C.
author_sort Lohfink, Anne M.
collection MIT
description We present an analysis of all XMM-Newton and Suzaku X-ray spectra of the nearby luminous Seyfert galaxy Fairall 9. Confirming previous analyses, we find robust evidence for a broad iron line associated with X-ray reflection from the innermost accretion disk. By fitting a spectral model that includes a relativistically ionized reflection component, we examine the constraints on the inclination of the inner accretion disk and the black hole spin, and the complications introduced by the presence of a photoionized emission line system. Employing multi-epoch fitting, we attempt to obtain robust and concordant measures of the accretion disk parameters. We also clearly see a soft X-ray excess in Fairall 9. During certain epochs, the soft excess can be described with the same disk reflection component that produces the iron line. However, there are epochs where an additional soft component is required. This can be attributed to either an additional highly ionized, strongly blurred disk reflection component or a new X-ray continuum component.
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spelling mit-1721.1/955002022-10-01T16:26:20Z THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9 Lohfink, Anne M. Reynolds, Christopher S. Miller, Jon M. Brenneman, Laura W. Mushotzky, Richard F. Nowak, Michael A. Fabian, Andrew C. MIT Kavli Institute for Astrophysics and Space Research Nowak, Michael A. We present an analysis of all XMM-Newton and Suzaku X-ray spectra of the nearby luminous Seyfert galaxy Fairall 9. Confirming previous analyses, we find robust evidence for a broad iron line associated with X-ray reflection from the innermost accretion disk. By fitting a spectral model that includes a relativistically ionized reflection component, we examine the constraints on the inclination of the inner accretion disk and the black hole spin, and the complications introduced by the presence of a photoionized emission line system. Employing multi-epoch fitting, we attempt to obtain robust and concordant measures of the accretion disk parameters. We also clearly see a soft X-ray excess in Fairall 9. During certain epochs, the soft excess can be described with the same disk reflection component that produces the iron line. However, there are epochs where an additional soft component is required. This can be attributed to either an additional highly ionized, strongly blurred disk reflection component or a new X-ray continuum component. 2015-02-25T13:15:16Z 2015-02-25T13:15:16Z 2012-09 2012-06 Article http://purl.org/eprint/type/JournalArticle 0004-637X 1538-4357 http://hdl.handle.net/1721.1/95500 Lohfink, Anne M., Christopher S. Reynolds, Jon M. Miller, Laura W. Brenneman, Richard F. Mushotzky, Michael A. Nowak, and Andrew C. Fabian. “THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9.” The Astrophysical Journal 758, no. 1 (September 26, 2012): 67. © 2012 The American Astronomical Society en_US http://dx.doi.org/10.1088/0004-637x/758/1/67 The Astrophysical Journal Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf IOP Publishing American Astronomical Society
spellingShingle Lohfink, Anne M.
Reynolds, Christopher S.
Miller, Jon M.
Brenneman, Laura W.
Mushotzky, Richard F.
Nowak, Michael A.
Fabian, Andrew C.
THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9
title THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9
title_full THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9
title_fullStr THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9
title_full_unstemmed THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9
title_short THE BLACK HOLE SPIN AND SOFT X-RAY EXCESS OF THE LUMINOUS SEYFERT GALAXY FAIRALL 9
title_sort black hole spin and soft x ray excess of the luminous seyfert galaxy fairall 9
url http://hdl.handle.net/1721.1/95500
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