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Jets from X-ray binaries
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Relativistic outflows, or `Jets', represent one of the most obvious, important and yet poorly-explained phenomena associated with accreting relativistic objects, including X-ray binaries. In the past decade we have observed highly relativistic flows, the resultant in-situ particle acceleration in the ISM, and begun to unearth the subtleties of the accretion -- outflow coupling on timescales from seconds to years. In this chapter I shall attempt, subjectively, to describe the state of research into jets from X-ray binaries as it stands at the beginning of 2003.
Forward citations
Cited by 10 Pith papers
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Spectropolarimetric detection of baryonic mass loading in a transient relativistic jet: application to the black hole X-ray binary Swift J1727.8$-$1613
Transient Faraday-complex spectropolarimetric structure detected during radio flaring of Swift J1727 implies internal Faraday rotation from electron-proton jet plasma with rotating mass ~10^21 g, a small fraction of a...
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The Mid-infrared Emitting Jet in the Black Hole V404 Cygni in Quiescence
Fast 21-micron flaring and a flat radio-to-mid-infrared spectrum show that the mid-infrared excess in the quiescent black hole binary V404 Cygni comes from a persistent relativistic jet.
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Observational Biases and Improved Modelling of Off-axis Relativistic Jets
Incorporating receding-jet non-detections tightens kinematic posteriors by >40% for MAXI J1535, while rest-frame modelling of MAXI J1820 shows strong observational bias against Γ0 ≳ 5 and receding ejecta.
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VLBI Diagnostics of Off-axis Jets in Radio Flares of Tidal Disruption Events
Synthetic VLBI images show that an off-axis jet in AT20118hyz would display superluminal centroid motion and a non-monotonic image aspect ratio, cleanly separating it from a delayed sub-relativistic outflow.
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The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.8$-$1613
In its 2023-2024 outburst, the black hole binary Swift J1727.8-1613 showed one of the most radio-quiet radio-X-ray tracks known, with X-ray spectral softening beginning just as the track changed slope.
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Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion
Time lag analysis using ICCF on GX 339-4 data reveals state-dependent radio-X-ray delays interpreted as evidence for magnetic field transport linking the inner accretion flow and jet.
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An Ejection Event Captured by VLBI During the Outburst of Swift J1727.8$-$1613
A 6-hour VLBI observation of Swift J1727.8-1613 reveals a fast-moving radio blob or pair of symmetric blobs, indicating a discrete ejection event during a state transition.
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4th TDAMM Workshop White Paper
A community white paper arguing TDAMM science is becoming follow-up-limited, and proposing pre-negotiated community observing plans with infrastructure, policy, and capability recommendations.
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GRMHD and GRRT Simulations of Black Hole Accretion: Flares, Precession, and Complex Spacetimes
Simulations of accreting black holes in standard and complex spacetimes indicate that magnetic geometry, quantum corrections, and binary dynamics influence flares, precession, photon rings, and multi-wavelength variab...
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SKAO and Gamma-Ray Synergies
Overview of synergies between SKA radio observations and gamma-ray facilities for studying transient, variable, and steady GeV-TeV sources.
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