REVIEW 10 cited by
Jets from X-ray binaries
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Jets from X-ray binaries
read the original abstract
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
-
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...
-
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.
-
Non-uniform particle injection into black hole jets by radiative magnetic reconnection
Pair production via radiative magnetic reconnection near spinning black holes supplies non-uniform plasma to jets at levels sufficient to explain M87 radio emission.
-
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.
-
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.
-
Isolating Broadband Radio Technosignatures (BRaTs): A Framework for Detecting Planetary-Scale Leakage
A tiered observational strategy is outlined to identify planetary-scale broadband radio technosignatures (BRaTs) from advanced civilizations up to 100 pc away using multi-parameter diagnostics to separate them from na...
-
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.
-
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...
-
Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion
Radio precedes X-ray Compton luminosity by ~3 days in the rising hard state but lags by ~8 days in the decaying hard state of GX 339-4, with inner magnetic field strength estimated from accretion rate and truncation r...
-
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.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.