Proof of principle X-ray reflection mass measurement of the black hole in H1743-322

Abstract

The black hole X-ray binary H1743-322 lies in a region of the Galaxy with high extinction, and therefore it has not been possible to make a dynamical mass measurement. In this paper we make use of a recent model which uses the X-ray reflection spectrum to constrain the ratio of the black hole mass to the source distance. By folding in a reported distance measurement, we are able to estimate the mass of the black hole to be $12\pm 2{\text{M}}_{\odot }$ ($1\sigma$ credible interval). We are then able to revise a previous disc continuum fitting estimate of black hole spin $a_{\ast }$ (previously relying on a population mass distribution) using our new mass constraint, finding $a_{\ast }=0.47\pm 0.10$. This work is a proof of principle demonstration of the method, showing it can be used to find the mass of black holes in X-ray binaries.

arXiv comment13 pages, 7 figures. Accepted for publication in MNRAS

References in corpus (70)

• On the Absorption of X-rays in the Interstellar Medium
• X-ray Properties of Black-Hole Binaries
• The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission
• Modelling the behaviour of accretion flows in X-ray binaries
• Compact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity
• Broad-band gamma-ray and X-ray spectra of NGC 4151 and their implications for physical processes and geometry
• Improved Reflection Models of Black-Hole Accretion Disks: Treating the Angular Distribution of X-rays
• The Black Hole Mass Distribution in the Galaxy
• The Spin of the Near-Extreme Kerr Black Hole GRS 1915+105
• Theoretical Black Hole Mass Distributions
• Spectral Properties of Accretion Disks Around Galactic and Extragalactic Black Holes
• Black Hole Spin in X-Ray Binaries: Observational Consequences
• The Mass Distribution of Stellar-Mass Black Holes
• X-ray reflected spectra from accretion disk models. III. A complete grid of ionized reflection calculations
• Low frequency QPO spectra and Lense-Thirring precession
• Multi-Temperature Blackbody Spectrum of a Thin Accretion Disk around a Kerr Black Hole: Model Computations and Comparison with Observations
• BlackCAT: A catalogue of stellar-mass black holes in X-ray transients
• GRS 1915+105 and the Disc-Jet Coupling in Accreting Black Hole Systems
• Irradiation of an Accretion Disc by a Jet: General Properties and Implications for Spin Measurements of Black Holes
• A review of quasi-periodic oscillations from black hole X-ray binaries: observation and theory
• The Mass of the Black Hole in Cygnus X-1
• WATCHDOG: A Comprehensive All-Sky Database of Galactic Black Hole X-ray Binaries
• Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets
• States and transitions in black-hole binaries
• Cygnus X-1 contains a 21-solar mass black hole -- implications for massive star winds
• Mass Measurements of Stellar and Intermediate Mass Black-Holes
• The observed velocity distribution of young pulsars
• A quasi-periodic modulation of the iron line centroid energy in the black hole binary H 1743-322
• X-ray Reflection Spectroscopy of the Black Hole GX 339-4: Exploring the Hard State with Unprecedented Sensitivity
• High-Density Effects in X-ray Reflection Models from Accretion Disks
• Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1
• The Distance, Inclination, and Spin of the Black Hole Microquasar H1743-322
• Towards precision measurements of accreting black holes using X-ray reflection spectroscopy
• Determination of Black Hole Masses in Galactic Black Hole Binaries using Scaling of Spectral and Variability Characteristics
• Alternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1
• NuSTAR and Swift observations of the very high state in GX 339-4: Weighing the black hole with X-rays
• High Density Reflection Spectroscopy: II. the Density of the Inner Black Hole Accretion Disc in AGN
• The evolution of a warped disc around a Kerr black hole
• No Time for Dead Time: Timing analysis of bright black hole binaries with NuSTAR
• A public relativistic transfer function model for X-ray reverberation mapping of accreting black holes
• Stellar Mass Black Holes and Ultraluminous X-Ray Sources
• The Soft-Excess in Mrk 509: Warm Corona or Relativistic Reflection?
• Measuring Black Hole Spin via the X-ray Continuum Fitting Method: Beyond the Thermal Dominant State
• Tomographic reflection modelling of quasi-periodic oscillations in the black hole binary H 1743-322
• High Density Reflection Spectroscopy I. A case study of GX~339-4
• Analysis of NuSTAR and Suzaku observations of Cyg X-1 in the hard state: evidence for a truncated disc geometry
• Doughnut strikes sandwich: the geometry of hot medium in accreting black hole X-ray binaries
• The soft component and the iron line as signatures of the disc inner radius in Galactic black hole binaries
• Estimation of Mass of Compact Object in H 1743-322 from 2010 and 2011 Outbursts using TCAF Solution and Spectral Index - QPO Frequency Correlation
• Apples and Oranges: Comparing black holes in X-ray binaries and gravitational-wave sources
• Solutions to the relativistic precession model
• A Systematic View of Ten New Black Hole Spins
• YNOGK: A new public code for calculating null geodesics in the Kerr spacetime
• Measurement of the absolute Crab flux with NuSTAR
• Phase-resolved spectroscopy of a quasi-periodic oscillation in the black hole X-ray binary GRS 1915+105 with NICER and NuSTAR
• Reflection Modeling of the Black Hole Binary 4U~1630$-$47: the Disk Density and Returning Radiation
• An Empirical Method for Improving the Quality of RXTE PCA Spectra
• A new model for QPOs in accreting black holes: application to the microquasar GRS 1915+105
• An X-ray reverberation mass measurement of Cygnus X-1
• The observed mass distribution of Galactic black hole LMXBs is biased against massive black holes
• Two major constraints on the inner radii of accretion disks
• Insight-HXMT, NuSTAR and INTEGRAL Data Show Disk Truncation in the Hard State of the Black-Hole X-Ray Binary MAXI J1820+070
• A strongly truncated inner accretion disk in the Rapid Burster
• Constraining the mass of the black hole GX 339-4 using spectro-temporal analysis of multiple outbursts
• Exploring the radial disc ionization profile of the black hole X-ray binary GRS 1915+105
• Effect of geometrically thin discs on precessing, thick flows: Relevance to type-C QPOs
• Constraints on mass, spin and magnetic field of microquasar H~1743-322 from observations of QPOs
• Spectro-timing study of GX 339-4 in a hard intermediate state
• High-density reflection spectroscopy of black hole X-ray binaries in the hard state
• On measuring the Hubble constant with X-ray reverberation mapping of active galactic nuclei

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