Dewangan, G. C. ; Mathur, S. ; Griffiths, R. E. ; Rao, A. R. (2008) X-ray emission from active galactic nuclei with intermediate-mass black holes The Astrophysical Journal, 689 (2). pp. 762-774. ISSN 0004-637X
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Official URL: http://iopscience.iop.org/0004-637X/689/2/762
Related URL: http://dx.doi.org/10.1086/591728
Abstract
We present a systematic X-ray study of eight active galactic nuclei (AGNs) with intermediate-mass black holes (MBH~ 8-95 × 104 M⊙) based on 12 XMM-Newton observations. The sample includes the two prototype AGNs in this class-NGC 4395 and POX 52 and six other AGNs discovered with the Sloan Digitized Sky Survey. These AGNs show some of the strongest X-ray variability, with the normalized excess variances being the largest and the power density break timescales being the shortest observed among radio-quiet AGNs. The excess-variance-luminosity correlation appears to depend on both the BH mass and the Eddington luminosity ratio. The break timescale-black hole mass relations for AGN with IMBHs are consistent with that observed for massive AGNs. We find that the FWHM of the Hβ /Hα line is uncorrelated with the BH mass, but shows strong anticorrelation with the Eddington luminosity ratio. Four AGNs show clear evidence for soft X-ray excess emission (kTin ~ 150-200 eV). X-ray spectra of three other AGNs are consistent with the presence of the soft excess emission. NGC 4395 with lowest L/LEdd lacks the soft excess emission. Evidently small black mass is not the primary driver of strong soft X-ray excess emission from AGNs. The X-ray spectral properties and optical-to-X-ray spectral energy distributions of these AGNs are similar to those of Seyfert 1 galaxies. The observed X-ray/UV properties of AGNs with IMBHs are consistent with these AGNs being low-mass extensions of more massive AGNs, those with high Eddington luminosity ratio looking more like narrow-line Seyfert 1 s and those with low L/LEdd looking more like broad-line Seyfert 1 galaxies.
Item Type: | Article |
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Source: | Copyright of this article belongs to University of Chicago Press. |
ID Code: | 85583 |
Deposited On: | 03 Mar 2012 14:52 |
Last Modified: | 19 May 2016 01:34 |
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