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The X-ray quasi-periodic oscillation (QPO) seen in RE J1034+396 is so far unique amongst AGN. Here we look at the another unique feature of RE J1034+396, namely its huge soft X-ray excess, to see if this is related in any way to the…

天体物理学 · 物理学 2015-05-13 Matthew Middleton , Chris Done , Martin Ward , Marek Gierlinski , Nick Schurch

Here we report an optical quasi-periodic oscillation (QPO) with a period of $\sim$134~day detected in g- and r-band light curves of a narrow-line Seyfert 1 galaxy TXS 1206+549 at redshift of 1.34 with the data from the Zwicky Transient…

高能天体物理现象 · 物理学 2023-12-13 Chongyang Ren , Sisi Sun , Pengfei Zhang

Black hole and neutron star X-ray binary systems routinely show quasi-periodic oscillations (QPOs) in their X-ray flux. Despite being strong, easily measurable signals, their physical origin has long remained elusive. However, recent…

高能天体物理现象 · 物理学 2021-06-30 Adam Ingram , Sara Motta

Long-standing optical quasi-periodic oscillations (QPOs) with periodicity of hundreds to thousands of days have been accepted as indicators for central sub-pc binary black hole systems (BBHs) in broad line active galactic nuclei (BLAGN).…

星系天体物理 · 物理学 2026-03-11 Liao GuiLin , Chen XingQian , Cheng PeiZhen , Zhang XueGuang

Kilohertz quasi-periodic oscillations or kHz QPOs occur on the orbital timescale of the inner accretion flow and may carry signatures of the physics of strong gravity (c$^{2}$ ~ GM/R) and possibly clues to constraining the neutron star…

高能天体物理现象 · 物理学 2018-06-26 Jon Troyer , Edward Cackett , Philippe Peille , Didier Barret

We present analysis of fast variability of Very Large Telescope/ISAAC (infra-red), \textit{XMM-Newton}/OM (optical) and EPIC-pn (X-ray), and RXTE/PCA (X-ray) observations of the black hole X-ray binary GX 339-4 in a rising hard state of its…

高能天体物理现象 · 物理学 2016-06-01 M. Kalamkar , P. Casella , P. Uttley , K. O'Brien , D. Russell , T. Maccarone , M. van der Klis , F. Vincentelli

We examine the nonlinear variability of quasi-periodic oscillations (QPOs) using the bicoherence, a measure of phase coupling at different Fourier frequencies. We analyse several observations of RXTE/PCA archival data of the black hole…

高能天体物理现象 · 物理学 2019-04-24 K. Arur , T. J. Maccarone

We have used archival RXTE PCA data to investigate timing and spectral characteristics of the transient XTE J1817-330. The data pertains to 160 PCA pointed observations made during the outburst period 2006, January 27 to August 2. A…

高能天体物理现象 · 物理学 2015-05-14 Jayashree Roy , P. C. Agrawal , B. Paul , K. Duorah

Motivated by the recent proposal that one can obtain quasi-periodic oscillations (QPOs) by photon echoes manifesting as non-trivial features in the autocorrelation function (ACF), we study the ACFs of the light curves of three accreting…

高能天体物理现象 · 物理学 2015-05-19 K. Fukumura , C. R. Shrader , J. W. Dong , D. Kazanas

Recent X-ray observations have revealed growing evidence of quasi-periodic oscillation (QPO) in the light curve of active galactic nuclei (AGNs), which may serve as a useful probe of black hole physics. In this work, we present a systematic…

高能天体物理现象 · 物理学 2021-11-12 Tong Bao , Zhiyuan Li

We present a model-independent analysis of the short-timescale energy dependence of low frequency quasi-periodic oscillations (QPOs) in the X-ray flux of GRS 1915+105. The QPO frequency in this source has previously been observed to depend…

高能天体物理现象 · 物理学 2016-03-16 Jakob van den Eijnden , Adam Ingram , Phil Uttley

We present the evolution of the phase lags associated with the type-C QPO in GX 339--4 during the rising phase of the 2006/2007 outburst. We find that the phase lags at the QPO frequency are always positive (hard), and show very different…

高能天体物理现象 · 物理学 2017-08-30 Liang Zhang , Yanan Wang , Mariano Mendez , Li Chen , Jinlu Qu , Diego Altamirano , Tomaso Belloni

We report the discovery of quasi-periodic oscillations (QPOs) at roughly 187 Hz and 150 Hz in the X-ray intensity of X-ray nova XTE J1859+226. The source was observed during a recent outburst with RXTE. Besides these high-frequency QPOs, we…

天体物理学 · 物理学 2007-05-23 Wei Cui , C. R. Shrader , C. A. Haswell , R. I. Hynes

Periodic outbursts are observed in many AGNs and usually explained with a supermassive black hole binary (SMBHB) scenario. However, multiple periods are observed in some AGNs and cannot be explained with it. Here we analyze the periodicity…

天体物理学 · 物理学 2008-11-26 F. K. Liu , G. Zhao , Xue-Bing Wu

We analyze the 11-year long-term light curve of the Radio-loud Narrow-line Seyfert 1 (NLSy1) galaxy J0849+5108 and the nearly simultaneous $\gamma$-ray data of the source. The data were obtained with the Owens Valley Radio Observatory 40-m…

高能天体物理现象 · 物理学 2021-06-23 Pengfei Zhang , Zhongxiang Wang

We compile observations of high-frequency quasi-periodic oscillations (QPOs) around black holes, both stellar and supermassive, and compare their positions in the parameter space of black hole mass, spin, and oscillation frequency. We find…

高能天体物理现象 · 物理学 2021-08-04 Krista Lynne Smith , Celia R. Tandon , Robert V. Wagoner

We present a detailed study of the 5 Hz quasi-periodic oscillation (QPO) recently discovered in the bright X-ray transient and black-hole candidate GRS 1739-278 (Borozdin & Trudolyubov 2000) during a Rossi X-ray Timing Explorer observation…

天体物理学 · 物理学 2009-11-06 Rudy Wijnands , Mariano Mendez , Jon M. Miller , Jeroen Homan

We analyzed RXTE/PCA and HEXTE data of the transient black hole binary GX 339-4, col- lected over a time span of eight years. We studied the properties and the behavior of low frequency quasi periodic oscillations (QPOs) as a function of…

高能天体物理现象 · 物理学 2015-05-30 S. Motta , T. Muñoz-Darias , P. Casella , T. Belloni , J. Homan

Quasi-periodic oscillations (QPOs) with frequencies from $\sim0.05$-$30$ Hz are a common feature in the X-ray emission of accreting black hole binaries. As the QPOs originate from the innermost accretion flow, they provide the opportunity…

高能天体物理现象 · 物理学 2016-11-23 J. van den Eijnden , A. Ingram , P. Uttley , S. E. Motta , T. M. Belloni , D. W. Gardenier

We propose a mechanism to explain the low-frequency QPOs observed in X-ray binary systems and AGNs. To achieve this, we perturbed stable accretion disks around Kerr and EGB black holes at different angular velocities, revealing…

高能天体物理现象 · 物理学 2024-05-27 Orhan Donmez