Tomographic reflection modelling of quasi-periodic oscillations in the black hole binary H 1743-322

Abstract

Accreting stellar mass black holes (BHs) routinely exhibit Type-C quasi-periodic oscillations (QPOs). These are often interpreted as Lense-Thirring precession of the inner accretion flow, a relativistic effect whereby the spin of the BH distorts the surrounding space-time, inducing nodal precession. The best evidence for the precession model is the recent discovery, using a long joint XMM-Newton and NuSTAR observation of H 1743-322, that the centroid energy of the iron fluorescence line changes systematically with QPO phase. This was interpreted as the inner flow illuminating different azimuths of the accretion disc as it precesses, giving rise to a blue/red shifted iron line when the approaching/receding disc material is illuminated. Here, we develop a physical model for this interpretation, including a self-consistent reflection continuum, and fit this to the same H 1743-322 data. We use an analytic function to parameterise the asymmetric illumination pattern on the disc surface that would result from inner flow precession, and find that the data are well described if two bright patches rotate about the disc surface. This model is preferred to alternatives considering an oscillating disc ionisation parameter, disc inner radius and radial emissivity profile. We find that the reflection fraction varies with QPO phase (3.5 sigma), adding to the now formidable body of evidence that Type-C QPOs are a geometric effect. This is the first example of tomographic QPO modelling, initiating a powerful new technique that utilizes QPOs in order to map the dynamics of accreting material close to the BH.

arXiv commentAccepted for publication in MNRAS

References in corpus (51)

• On the Absorption of X-rays in the Interstellar Medium
• Modelling the behaviour of accretion flows in X-ray binaries
• Broad-band gamma-ray and X-ray spectra of NGC 4151 and their implications for physical processes and geometry
• Lense-Thirring Precession and QPOs in Low Mass X-Ray Binaries
• Improved Reflection Models of Black-Hole Accretion Disks: Treating the Angular Distribution of X-rays
• The Black Hole Mass Distribution in the Galaxy
• Going with the flow: can the base of jets subsume the role of compact accretion disk coronae?
• The Mass Distribution of Stellar-Mass Black Holes
• X-ray reflected spectra from accretion disk models. III. A complete grid of ionized reflection calculations
• X-ray reverberation around accreting black holes
• Low frequency QPO spectra and Lense-Thirring precession
• The ABC of low-frequency quasi-periodic oscillations in Black-Hole Candidates: analogies with Z-sources
• Global General Relativistic MHD Simulation of a Tilted Black-Hole Accretion Disk
• Aligning spinning black holes and accretion discs
• Understanding X-ray reflection emissivity profiles in AGN: Locating the X-ray source
• Thermal Instability and Photoionized X-ray Reflection in Accretion Disks
• A Fast New Public Code for Computing Photon Orbits in a Kerr Spacetime
• 'Stable' QPOs and Black Hole Properties from Diskoseismology
• The Complex Phase Lag Behavior of the 3-12 Hz Quasi-Periodic Oscillations during the Very High State of XTE J1550-564
• A quasi-periodic modulation of the iron line centroid energy in the black hole binary H 1743-322
• Geometrical constraints on the origin of timing signals from black holes
• High- and low-frequency quasi-periodic oscillations in the X-ray light curves of the black hole transient H1743-322
• Determination of Black Hole Masses in Galactic Black Hole Binaries using Scaling of Spectral and Variability Characteristics
• On the determination of the spin of the black hole in Cyg X-1 from X-ray reflection spectra
• Determination of the X-ray reflection emissivity profile of 1H 0707-495
• Modelling variability in black hole binaries: linking simulations to observations
• A Precessing Ring Model for Low-Frequency Quasi-periodic Oscillations
• Variability of X-ray binaries from an oscillating hot corona
• Phase-resolved X-ray spectroscopy of the millisecond pulsar SAX J1808.4-3658
• Light curves and polarization of accretion- and nuclear-powered millisecond pulsars
• The truncated and evolving inner accretion disc of the black hole GX 339-4
• Spectral and Fourier analyses of X-ray QPO in accreting black holes
• A unified Lense-Thirring precession model for optical and X-ray quasi-periodic oscillations in black hole binaries
• The soft component and the iron line as signatures of the disc inner radius in Galactic black hole binaries
• Phase-resolved spectroscopy of low frequency quasi-periodic oscillations in GRS 1915+105
• Inclination-dependent spectral and timing properties in transient black hole X-ray binaries
• Effective Inner Radius of Tilted Black Hole Accretion Disks
• Phase-Resolved Spectroscopy of Type B Quasi-Periodic Oscillations in GX 339-4
• Solutions to the relativistic precession model
• A Broad Iron Line in LMC X-1
• Evidence for a Link Between Fe K-alpha Emission Line Strength and QPO Phase in a Black Hole
• Can the soft excess in AGN originate from disc reflection?
• Origin of the X-ray disc-reflection steep radial emissivity
• The effect of frame dragging on the iron K alpha line in X-ray binaries
• Probing the origin of quasi-periodic oscillations: the short-timescale evolution of phase lags in GRS 1915+105
• The reverberation lag in the low mass X-ray binary H1743-322
• An imperfect double: probing the physical origin of the low-frequency QPO and its harmonic in black hole binaries
• Role of emission angular directionality in spin determination of accreting black holes with broad iron line
• Using XMM-Newton to study the energy dependent variability of H 1743-322 during its 2014 outburst
• Doppler disc tomography applied to low mass AGN spin
• Pulse-phase resolved spectroscopy of continuum and reflection in SAX J1808.4-3658

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• Upper-twin-peak quasiperiodic oscillation in x-ray binaries and the energy from tidal circularization of relativistic orbits
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• A Phase-resolved View of the Low-frequency Quasiperiodic Oscillations from the Black Hole Binary MAXI J1820+070
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• Black-hole X-ray binary Swift J1727.8$-$1613 shows simultaneous Type-B and Type-C quasi-periodic oscillations across the hard-intermediate and soft-intermediate states
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