Thermally-Driven Disc Winds as a Mechanism for X-ray Irradiation Heating in Black Hole X-ray Binaries: The Case Study of GX339-4

Abstract

X-ray irradiation heating of accretion discs in black hole X-ray binaries (BHXBs) plays a key role in regulating their outburst cycles. However, despite decades of theoretical and observational efforts, the physical mechanism(s) responsible for irradiating these discs remains largely unknown. We have built an observationally-based methodology to estimate the strength of irradiation of BHXB discs by combining multiwavelength X-ray and optical/IR data throughout transient outbursts. We apply this to $\sim 15$ yrs of activity in the Galactic BHXB GX339$-$4. Our findings suggest that the irradiation heating required by the optical data is large in this system. Direct illumination of the outer disc does not produce sufficient irradiation, but this should also produce a thermal-radiative wind which adds to the irradiation heating by scattering flux down onto the disc. However, analytic estimates of X-ray illumination from scattering in the wind is still not sufficient to produce the observed heating, even in combination with direct illumination. Either the analytic thermal-radiative wind models are underestimating the effect of the wind, or there are additional scattering mechanisms at work, such as magnetically-driven outflows, acting to increase the optical/IR flux. While wind-driven irradiation is likely a common feature among long-period BHXBs, fully understanding the driving mechanism(s) behind such a wind will require radiation-hydrodynamic simulations.

arXiv comment34 pages, 7 figures, supplementary figures included in appendices, accepted for publication in MNRAS

References in corpus (74)

• emcee: The MCMC Hammer
• Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs
• Modelling the behaviour of accretion flows in X-ray binaries
• A universal radio/X-ray correlation in low/hard state black hole binaries
• The Black Hole Mass Distribution in the Galaxy
• The Properties of X-Ray and Optical Light Curves of X-Ray Novae
• Powerful jets from black hole X-ray binaries in Low/Hard X-ray states
• Radio / X-ray correlation in the low/hard state of GX 339--4
• Ubiquitous equatorial accretion disc winds in black hole soft states
• The disc instability model for X-ray transients: evidence for truncation and irradiation
• WATCHDOG: A Comprehensive All-Sky Database of Galactic Black Hole X-ray Binaries
• Jets in neutron star X-ray binaries: a comparison with black holes
• X-ray irradiation in low mass binary systems
• GX 339-4: the distance, state transitions, hysteresis and spectral correlations
• A Long, Hard Look at the Low-Hard State in Accreting Black Holes
• Near-infrared synchrotron emission from the compact jet of GX339-4
• Dynamical Evidence for a Black Hole in GX 339-4
• Global optical/infrared - X-ray correlations in X-ray binaries: quantifying disc and jet contributions
• Broad-band X-ray/gamma-ray spectra and binary parameters of GX 339-4 and their astrophysical implications
• Multi-wavelength observations of the 2002 outburst of GX 339-4: two patterns of X-ray-optical/near-infrared behavior
• X-ray Reflection Spectroscopy of the Black Hole GX 339-4: Exploring the Hard State with Unprecedented Sensitivity
• Simultaneous Chandra and RXTE Spectroscopy of the Microquasar H~1743-322: Clues to Disk Wind and Jet Formation from a Variable Ionized Outflow
• Chandra/HETGS Spectroscopy of the Galactic Black Hole GX 339-4: A Relativistic Iron Line and Evidence for a Seyfert-like Warm Absorber
• A systematic look at the Very High and Low/Hard state of GX 339-4: Constraining the black hole spin with a new reflection model
• The Distance and Interstellar Sight Line to GX339-4
• A unified accretion-ejection paradigm for Black Hole X-ray Binaries
• Reprocessing of X-rays in the outer accretion disc of the black hole binary XTE J1817--330
• Potential Kick Velocity distribution of black hole X-ray binaries and implications for natal kicks
• Revisiting a fundamental test of the disc instability model for X-ray binaries
• NuSTAR and Swift observations of the very high state in GX 339-4: Weighing the black hole with X-rays
• Rapid optical and X-ray timing observations of GX 339-4: multi-component optical variability in the low/hard state
• Jet spectral breaks in black hole X-ray binaries
• A transient large-scale relativistic radio jet from GX 339-4
• The infrared/X-ray correlation of GX 339-4: Probing hard X-ray emission in accreting black holes
• The Evolving Accretion Disc in the Black Hole X-ray Transient XTE J1859+226
• Strong disc winds traced throughout outbursts in black-hole X-ray binaries
• The mass function of GX 339-4 from spectroscopic observations of its donor star
• The complex accretion geometry of GX 339-4 as seen by NuSTAR and Swift
• A Swift survey of accretion onto stellar-mass black holes
• Accretion disc outbursts: a new version of an old model
• A re--analysis of the iron line in the XMM-Newton data from the low/hard state in GX339--4
• The truncated and evolving inner accretion disc of the black hole GX 339-4
• The Optical and Ultraviolet Spectral Energy Distributions of Short Period Black Hole X-ray Transients in Outburst
• Inclination and relativistic effects in the outburst evolution of black hole transients
• Spectral analysis of the XMM-Newton data of GX 339-4 in the low/hard state: disc truncation and reflection
• Optical and Near Infrared Monitoring of the Black-Hole X-ray Binary GX 339-4 During 2002-2010
• Why Low-Mass Black-Hole Binaries Are Transient
• Testing the disk instability model of cataclysmic variables
• The evolution of GX 339-4 in the low-hard state as seen by NuSTAR and Swift
• Near-infrared jet emission in the microquasar XTE J1550-564
• Thermal Winds in Stellar Mass Black Hole and Neutron Star Binary Systems
• Disc instability models for X-ray transients: evidence for evaporation and low alpha-viscosity ?
• Multiwavelength Observations of A0620-00 in Quiescence
• A unified accretion-ejection paradigm for black hole X-ray binaries. III. Spectral signatures of hybrid disk configurations
• A unified accretion-ejection paradigm for black hole X-ray binaries. II. Observational signatures of jet-emitting disks
• XMM-Newton observations reveal the disappearance of the wind in 4U 1630-47
• Coronae and Winds from Irradiated Disks in X-ray binaries
• A unified accretion-ejection paradigm for black hole X-ray binaries. IV. Replication of the 2010--2011 activity cycle of GX 339-4
• Optical Lightcurves of the Black Hole Binaries GRS 1124-68 and A0620-00 in Outburst: the Importance of Irradiation
• The effects of thermodynamic stability on wind properties in different low mass black hole binary states
• Understanding X-ray Irradiation in Low-Mass X-ray Binaries directly from their Light-Curves
• SW Sextantis in an excited, low state
• Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst
• The thermal-radiative wind in low mass X-ray binary H 1743-322; Radiation hydrodynamic simulations
• The impact of thermal winds on the outburst lightcurves of black hole X-ray binaries
• The Case for Massive, Evolving Winds in Black Hole X-ray Binaries
• The thermal-radiative wind in low mass X-ray binary H 1743-322: II. iron line predictions from Monte Carlo radiation transfer
• Time-Evolved X-ray Irradiation during the 1999$-$2000 Outburst of the Black-Hole Binary XTE J1859+226
• Determination of the turbulent parameter in the accretion disks: effects of self-irradiation in 4U 1543-47 during the 2002 outburst
• Systematic spectral analysis of GX 339-4: influence of Galactic background and reflection models
• Black-Hole X-Ray Transients: The Effect of Irradiation on Time-Dependent Accretion Disk Structure
• Application of the Thermal Wind Model to Absorption Features in the Black Hole X-ray Binary H 1743-322
• The Curious Case of Swift J1753.5-0127: A Black Hole Low-mass X-ray Binary Analogue to Z Cam Type Dwarf Novae
• Observational tests of the picture of disk accretion

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