Investigating the disc-jet coupling in accreting compact objects using the black hole candidate Swift J1753.5-0127

Abstract

In studies of accreting black holes in binary systems, empirical relations have been proposed to quantify the coupling between accretion processes and ejection mechanisms. These processes are probed respectively by means of X-ray and radio/optical-infrared observations. The relations predict, given certain accretion conditions, the expected energy output in the form of a jet. We investigated this coupling by studying the black hole candidate Swift J1753.5-0127, via multiwavelength coordinated observations over a period of ~4 years. We present the results of our campaign showing that, all along the outburst, the source features a jet that is fainter than expected from the empirical correlation between the radio and the X-ray luminosities in hard spectral state. Because the jet is so weak in this system the near-infrared emission is, unusually for this state and luminosity, dominated by thermal emission from the accretion disc. We briefly discuss the importance and the implications of a precise determination of both the slope and the normalisation of the correlations, listing some possible parameters that broadband jet models should take into account to explain the population of sources characterized by a dim jet. We also investigate whether our data can give any hint about the nature of the compact object in the system, since its mass has not been dynamically measured.

Accepted for publication in MNRAS

References in corpus (29)

• X-ray Properties of Black-Hole Binaries
• Radio-Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications
• A Long, Hard Look at the Low-Hard State in Accreting Black Holes
• Global optical/infrared - X-ray correlations in X-ray binaries: quantifying disc and jet contributions
• A radio-emitting outflow in the quiescent state of A0620-00: implications for modelling low-luminosity black hole binaries
• Accretion states and radio loudness in Active Galactic Nuclei: analogies with X-ray binaries
• Jet-dominated advective systems: radio and X-ray luminosity dependence on the accretion rate
• The 2003 Outburst of the X-ray Transient H 1743-322: Comparisons with the Black Hole Microquasar XTE J1550-564
• Fast infrared variability from a relativistic jet in GX 339-4
• A Prominent Accretion Disk in the Low-Hard State of the Black Hole Candidate SWIFT J1753.5-0127
• Revisiting the radio/X-ray flux correlation in the black hole V404 Cyg: from outburst to quiescence
• The synchrotron boiler and the spectral states of black hole binaries
• The variability plane of accreting compact objects
• The spectral energy distribution of quiescent black hole X-ray binaries: new constraints from Spitzer
• The origin and fate of short-period low-mass black-hole binaries
• Swift J1753.5-0127: The Black Hole Candidate with the shortest orbital period
• A Model for Emission from Jets in X-ray Binaries: Consequences of a Single Acceleration Episode
• Tracing the jet contribution to the mid-IR over the 2005 outburst of GRO J1655-40 via broadband spectral modeling
• XMM-Newton observation of a spectral state transition in the peculiar radio/X-ray/gamma-ray source LS I +61 303
• Multiwavelength spectral and high time resolution observations of SWIFT J1753.5-0127: new activity?
• Parallel tracks in infrared versus X-ray emission in black hole X-ray transient outbursts: a hysteresis effect?
• Zooming in on a sleeping giant: milliarcsecond HSA imaging of the black hole binary V404 Cyg in quiescence
• On the Radio/X-ray Correlation in Microquasars
• RXTE observations of the Low/Hard State X-ray Outburst of the new x-ray transient SWIFT J1753.5-0127
• Disentangling jet and disc emission from the 2005 outburst of XTE J1118+480
• Simultaneous INTEGRAL and RXTE observations of the accreting millisecond pulsar HETE J1900.1-2455
• ADAFs, accretion discs and outbursts in compact binaries
• Outliers from the mainstream: how a massive star can produce a gamma-ray burst
• X-ray Spectral and timing properties of the black hole x-ray transient Swift J1753.5-0127

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• MAXI J1659-152: The shortest orbital period black-hole transient in outburst
• The 1.4 GHz radio properties of hard X-ray selected AGN
• A new fundamental plane for radiatively efficient black-hole sources
• A complex state transition from the black hole candidate Swift J1753.5-0127
• A deep radio survey of hard state and quiescent black hole X-ray binaries
• The relation between radio and X-ray luminosity of black hole binaries: affected by inner cool disks?
• Radio-loudness in black hole transients: evidence for an inclination effect
• Bright mini-outburst ends the 12-year long activity of the black hole candidate Swift J1753.5-0127
• On the nature of the "radio quiet" black hole binaries
• Accretion Flow Properties of Swift J1753.5-0127 during its 2005 outburst
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• Properties of X-ray Flux of Jets During 2005 Outburst of Swift J1753.5-0127 Using TCAF Solution
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• Different X-ray spectral evolution for black hole X-ray binaries in dual tracks of radio-X-ray correlation
• Swift Observations of MAXI J1659-152: A Compact Binary with a Black Hole Accretor
• The radio/X-ray correlation in X-ray binaries - Insights from a hard X-ray perspective
• Discovery of correlated optical/X-ray quasi-periodic oscillations in black hole binary SWIFT J1753.5-0127
• Up and Down the Black Hole Radio/X-ray Correlation: the 2017 mini-outbursts from Swift J1753.5-0127
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• The Accreting Black Hole Swift J1753.5-0127 from Radio to Hard X-Ray
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• The Megasecond Chandra X-Ray Visionary Project Observation of NGC 3115 (II): properties of point sources
• The origin of UV/optical emission in the black hole low-mass X-ray binary Swift J1753.5-0127
• Modeling the Spectrum of IGR J17177-3656
• Accretion Disc-Jet Couplings in X-ray Binaries
• A 2.5-dimensional viscous, resistive, advective magnetized accretion-outflow coupling in black hole systems: A higher order polynomial approximation. I
• Long-Term Monitoring of the Black Hole Candidate Swift J1753.5-0127 with INTEGRAL/SPI