The X-ray Binary analogy to the first AGN QPO

被引：1
作者：
Middleton, M. [1 ]
Done, C. [1 ]
Gierlinski, M. [1 ]
机构：
[1] Univ Durham, Durham DH1 3LE, England
来源：
X-RAY ASTRONOMY-2009: PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES, PROCEEDINGS | 2010年 / 1248卷
关键词：
Black holes; AGN; Seyferts; QPO; ACTIVE GALACTIC NUCLEI; QUASI-PERIODIC OSCILLATIONS; ACCRETING BLACK-HOLES; VARIABILITY; SPECTRA; ORIGIN; GALAXY; EXCESS; STATE; RXTE;
D O I：
10.1063/1.3475248
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We examine the different QPOs seen in X-ray Binaries for an analogous signal to the first AGN QPO. Simple mass scaling rules out the low-frequency and standard high-frequency QPOs. However, the rather unique 67Hz QPO of GRS 1915+105 scales to imply the source is accreting at around Eddington as supported by the SED. The 67Hz QPO is seen when GRS 1915+105 is in a very similar spectral state to that of RE J1034+396 and the power spectrum continuum slopes below the QPOs, are consistent. The difference in normalisation is suggested to be intrinsic and subsequent bandpass corrections yield consistent values.
引用
收藏
页码：325 / 328
页数：4
相关论文
共 50 条
[31]   The X-ray disc/wind degeneracy in AGN [J].
Parker, M. L. ;
Matzeu, G. A. ;
Matthews, J. H. ;
Middleton, M. J. ;
Dauser, T. ;
Jiang, J. ;
Joyce, A. M. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 513 (01) :551-572
[32]   Dependence of clustering of X-ray AGN on obscuration [J].
Koutoulidis, L. ;
Georgantopoulos, I. ;
Mountrichas, G. ;
Plionis, M. ;
Georgakakis, A. ;
Akylas, A. ;
Rovilos, E. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 481 (03) :3063-3069
[33]   AGN UNIFICATION AT z ∼ 1: u - R COLORS AND GRADIENTS IN X-RAY AGN HOSTS [J].
Ammons, S. Mark ;
Rosario, David J. V. ;
Koo, David C. ;
Dutton, Aaron A. ;
Melbourne, Jason ;
Max, Claire E. ;
Mozena, Mark ;
Kocevski, Dale D. ;
McGrath, Elizabeth J. ;
Bouwens, Rychard J. ;
Magee, Daniel K. .
ASTROPHYSICAL JOURNAL, 2011, 740 (01)
[34]   Exceptional AGN long-timescale X-ray variability: The case of PHL 1092 [J].
Miniutti, G. ;
Brandt, W. N. ;
Schneider, D. P. ;
Fabian, A. C. ;
Gallo, L. C. ;
Boller, Th. .
TIDAL DISRUPTION EVENTS AND AGN OUTBURSTS, 2012, 39
[35]   Simultaneous X-ray and optical spectroscopy of V404 Cygni supports the multi-phase nature of X-ray binary accretion disc winds [J].
Munoz-Darias, Teo ;
Ponti, Gabriele .
ASTRONOMY & ASTROPHYSICS, 2022, 664
[36]   X-ray luminosity functions of different morphological and X-ray type AGN populations [J].
Povic, M. ;
Perez Garcia, A. M. ;
Sanchez-Portal, M. ;
Bongiovanni, A. ;
Cepa, J. ;
Fernandez Lorenzo, M. ;
Lara-Lopez, M. A. ;
Gallego, J. ;
Ederoclite, A. ;
Marquez, I. ;
Masegosa, J. ;
Alfaro, E. ;
Castaneda, H. ;
Gonzalez-Serrano, J. I. ;
Gonzalez, J. J. .
ASTRONOMISCHE NACHRICHTEN, 2013, 334 (03) :288-299
[37]   BAT AGN spectroscopic survey - XV: the high frequency radio cores of ultra-hard X-ray selected AGN [J].
Smith, Krista Lynne ;
Mushotzky, Richard F. ;
Koss, Michael ;
Trakhtenbrot, Benny ;
Ricci, Claudio ;
Wong, O. Ivy ;
Bauer, Franz E. ;
Ricci, Federica ;
Vogel, Stuart ;
Stern, Daniel ;
Powell, Meredith C. ;
Urry, C. Meg ;
Harrison, Fiona ;
Mejia-Restrepo, Julian ;
Oh, Kyuseok ;
Baek, Junhyun ;
Chung, Aeree .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 492 (03) :4216-4234
[38]   Re-observing the NLS1 galaxy RE J1034+396-II. New insights on the soft X-ray excess, QPO, and the analogy with GRS 1915+105 [J].
Jin, Chichuan ;
Done, Chris ;
Ward, Martin .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 500 (02) :2475-2495
[39]   X-ray spectral evolution in an X-ray changing-look AGN NGC 1365 with variable column density [J].
Liu, Hao ;
Wu, Qing-Wen ;
Xue, Yong-Quan ;
Wang, Ting-Gui ;
Yang, Jun ;
Guo, Heng-Xiao ;
He, Zhi-Cheng .
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2021, 21 (08)
[40]   Relation between spectral changes and the presence of the lower kHz QPO in the neutron star low-mass X-ray binary 4U 1636-53 [J].
Zhang, Guobao ;
Mendez, Mariano ;
Sanna, Andrea ;
Ribeiro, Evandro M. ;
Gelfand, Joseph D. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 465 (04) :5003-5010
12345