THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33

We present results from Suzaku and Swift observations of the nearby radio galaxy 3C 33, and investigate the nature of absorption, reflection, and jet production in this source. We model the 0.5-100 keV nuclear continuum with a power law that is transmitted either through one or more layers of pc-sca...

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Main Authors: Evans, Daniel A., Reeves, J. N., Hardcastle, M. J., Kraft, Ralph P., Lee, J. C., Virani, S. N.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: Institute of Physics/American Astronomical Society 2015
Online Access:http://hdl.handle.net/1721.1/96214
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author Evans, Daniel A.
Reeves, J. N.
Hardcastle, M. J.
Kraft, Ralph P.
Lee, J. C.
Virani, S. N.
author2 MIT Kavli Institute for Astrophysics and Space Research
author_facet MIT Kavli Institute for Astrophysics and Space Research
Evans, Daniel A.
Reeves, J. N.
Hardcastle, M. J.
Kraft, Ralph P.
Lee, J. C.
Virani, S. N.
author_sort Evans, Daniel A.
collection MIT
description We present results from Suzaku and Swift observations of the nearby radio galaxy 3C 33, and investigate the nature of absorption, reflection, and jet production in this source. We model the 0.5-100 keV nuclear continuum with a power law that is transmitted either through one or more layers of pc-scale neutral material, or through a modestly ionized pc-scale obscurer. The standard signatures of reflection from a neutral accretion disk are absent in 3C 33: there is no evidence of a relativistically blurred Fe Kα emission line, and no Compton reflection hump above 10 keV. We find the upper limit to the neutral reflection fraction is R < 0.41 for an e-folding energy of 1 GeV. We observe a narrow, neutral Fe Kα line, which is likely to originate at least 2000 R [subscript s] from the black hole. We show that the weakness of reflection features in 3C 33 is consistent with two interpretations: either the inner accretion flow is highly ionized, or the black-hole spin configuration is retrograde with respect to the accreting material.
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spelling mit-1721.1/962142022-10-01T00:40:15Z THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33 Evans, Daniel A. Reeves, J. N. Hardcastle, M. J. Kraft, Ralph P. Lee, J. C. Virani, S. N. MIT Kavli Institute for Astrophysics and Space Research Evans, Daniel A. We present results from Suzaku and Swift observations of the nearby radio galaxy 3C 33, and investigate the nature of absorption, reflection, and jet production in this source. We model the 0.5-100 keV nuclear continuum with a power law that is transmitted either through one or more layers of pc-scale neutral material, or through a modestly ionized pc-scale obscurer. The standard signatures of reflection from a neutral accretion disk are absent in 3C 33: there is no evidence of a relativistically blurred Fe Kα emission line, and no Compton reflection hump above 10 keV. We find the upper limit to the neutral reflection fraction is R < 0.41 for an e-folding energy of 1 GeV. We observe a narrow, neutral Fe Kα line, which is likely to originate at least 2000 R [subscript s] from the black hole. We show that the weakness of reflection features in 3C 33 is consistent with two interpretations: either the inner accretion flow is highly ionized, or the black-hole spin configuration is retrograde with respect to the accreting material. United States. National Aeronautics and Space Administration (grant number NNX08AI59G) Royal Society (Great Britain) (Research Fellowship) 2015-03-27T15:54:17Z 2015-03-27T15:54:17Z 2010-02 2009-04 Article http://purl.org/eprint/type/JournalArticle 0004-637X 1538-4357 http://hdl.handle.net/1721.1/96214 Evans, D. A., J. N. Reeves, M. J. Hardcastle, R. P. Kraft, J. C. Lee, and S. N. Virani. “THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33.” The Astrophysical Journal 710, no. 1 (January 22, 2010): 859–868. © 2010 American Astronomical Society. en_US http://dx.doi.org/10.1088/0004-637x/710/1/859 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 Institute of Physics/American Astronomical Society American Astronomical Society
spellingShingle Evans, Daniel A.
Reeves, J. N.
Hardcastle, M. J.
Kraft, Ralph P.
Lee, J. C.
Virani, S. N.
THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33
title THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33
title_full THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33
title_fullStr THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33
title_full_unstemmed THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33
title_short THE HARD X-RAY VIEW OF REFLECTION, ABSORPTION, AND THE DISK-JET CONNECTION IN THE RADIO-LOUD AGN 3C 33
title_sort hard x ray view of reflection absorption and the disk jet connection in the radio loud agn 3c 33
url http://hdl.handle.net/1721.1/96214
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