Modeling the Fe K Line Profiles in Type I Active Galactic Nuclei with a Compton-thick Disk Wind
作者： L Miller , A R Patrick , K S Long , M M Tatum , J N Reeves
DOI: 10.1088/0004-637X/752/2/94
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摘要: 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 all contain moderately broad components Fe K-shell emission and are ideal candidates for testing the applicability Compton-thick accretion disk wind model to active galactic nucleus (AGN) components. Viewing angles through allow observer see absorption signature gas, whereas face-on viewing scattered light from wind. find Fe K line profiles well described solar abundances, arising tens hundreds gravitational radii central black hole. Further, fits require neutral component Fe Kα is too narrow arise inner part wind, likely comes more distant reprocessing region. Our study demonstrates can profound effect on observed spectrum an AGN, even when system not viewed flow.
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Jong‐Hak Woo, C. Megan Urry, Active Galactic Nucleus Black Hole Masses and Bolometric Luminosities The Astrophysical Journal. ,vol. 579, pp. 530- 544 ,(2002) , 10.1086/342878
L. Miller, I. M. George, I. M. George, J. N. Reeves, J. N. Reeves, S. B. Kraemer, S. B. Kraemer, B. Wingert, T. J. Turner, T. J. Turner, The variable X-ray spectrum of Markarian 766 - I. Principal components analysis Astronomy and Astrophysics. ,vol. 463, pp. 131- 143 ,(2007) , 10.1051/0004-6361:20066548
M. Guainazzi, S. Bianchi, G. Matt, M. Dadina, J. Kaastra, J. Malzac, G. Risaliti, The final verdict by XMM-Newton: the X-ray obscured Seyfert galaxy NGC5506 has a broad Fe K-alpha line arXiv: Cosmology and Nongalactic Astrophysics. ,(2010) , 10.1111/J.1365-2966.2010.16805.X
J. N. Reeves, P. T. O'Brien, M. J. Ward, A Massive X-Ray Outflow from the Quasar PDS 456 The Astrophysical Journal. ,vol. 593, ,(2003) , 10.1086/378218
L. Miller, T. J. Turner, J. N. Reeves, A. Lobban, S. B. Kraemer, D. M. Crenshaw, Spectral variability and reverberation time delays in theSuzakuX-ray spectrum of NGC 4051 Monthly Notices of the Royal Astronomical Society. ,vol. 403, pp. 196- 210 ,(2010) , 10.1111/J.1365-2966.2009.16149.X
Kenneth A. Pounds, Andrew R. King, Andrew R. King, Black hole winds Monthly Notices of the Royal Astronomical Society. ,vol. 345, pp. 657- 659 ,(2003) , 10.1046/J.1365-8711.2003.06980.X
C. Knigge, J. A. Woods, J. E. Drew, The application of Monte Carlo methods to the synthesis of spectral line profiles arising from accretion disc winds Monthly Notices of the Royal Astronomical Society. ,vol. 273, pp. 225- 248 ,(1995) , 10.1093/MNRAS/273.2.225
A. De Rosa, A. Turner, A. J. Young, A long hard look at MCG–6-30-15 with XMM-Newton Monthly Notices of the Royal Astronomical Society. ,vol. 335, ,(2002) , 10.1046/J.1365-8711.2002.05740.X
G. Risaliti, S. Bianchi, G. Matt, A. Baldi, M. Elvis, G. Fabbiano, A. Zezas, Highly Ionized Iron Absorption Lines from Outflowing Gas in the X-Ray Spectrum of NGC 1365 The Astrophysical Journal. ,vol. 630, pp. 129- ,(2005) , 10.1086/491646
C. J. Grier, B. M. Peterson, R. W. Pogge, K. D. Denney, M. C. Bentz, Paul Martini, S. G. Sergeev, S. Kaspi, Y. Zu, C. S. Kochanek, B. J. Shappee, K. Z. Stanek, C. Araya Salvo, T. G. Beatty, J. C. Bird, D. J. Bord, G. A. Borman, X. Che, C. Chen, S. A. Cohen, M. Dietrich, V. T. Doroshenko, Yu. S. Efimov, N. Free, I. Ginsburg, C. B. Henderson, Keith Horne, A. L. King, K. Mogren, M. Molina, A. M. Mosquera, S. V. Nazarov, D. N. Okhmat, O. Pejcha, S. Rafter, J. C. Shields, J. Skowron, D. M. Szczygiel, M. Valluri, J. L. van Saders, A REVERBERATION LAG FOR THE HIGH-IONIZATION COMPONENT OF THE BROAD-LINE REGION IN THE NARROW-LINE SEYFERT 1 Mrk 335 The Astrophysical Journal. ,vol. 744, pp. 4- 8 ,(2012) , 10.1088/2041-8205/744/1/L4