An overview of jets and outflows in stellar mass black holes

Abstract

In this book chapter, we will briefly review the current empirical understanding of the relation between accretion state and and outflows in accreting stellar mass black holes. The focus will be on the empirical connections between X-ray states and relativistic (`radio') jets, although we are now also able to draw accretion disc winds into the picture in a systematic way. We will furthermore consider the latest attempts to measure/order jet power, and to compare it to other (potentially) measurable quantities, most importantly black hole spin.

arXiv commentAccepted for publication in Space Science Reviews. Also to appear in the Space Sciences Series of ISSI - The Physics of Accretion on to Black Holes (Springer Publisher)

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• Disentangling jet and disc emission from the 2005 outburst of XTE J1118+480
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• What is on Tap? The Role of Spin in Compact Objects and Relativistic Jets
• Using SKA to observe relativistic jets from X-ray binary systems
• Observations and models of slow solar wind with Mg9+ ions in quiescent streamers

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• The Sardinia Radio Telescope: From a Technological Project to a Radio Observatory
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• Accretion Flow Dynamics During 1999 Outburst of XTE J1859+226 - Modeling of Broadband Spectra and Constraining the Source Mass
• Jets, disc-winds and oscillations in general relativistic, magnetically driven flows around black hole
• Observations of a black hole X-ray binary indicate formation of a magnetically arrested disk
• Estimation of mass outflow rates from dissipative accretion disc around rotating black holes
• Giant Metrewave Radio Telescope monitoring of the black hole X-ray binary, V404 Cygni, during its June 2015 outburst
• The luminosity dependence of thermally-driven disc winds in low-mass X-ray binaries
• High-precision optical polarimetry of the accreting black hole V404 Cyg during the June 2015 outburst
• Parsec-scale radio morphology and variability of a changing-look AGN: the case of Mrk 590
• Evolving optical polarisation of the black hole X-ray binary MAXI J1820+070
• Are Low-Frequency Quasi-Periodic Oscillations seen in accretion flows the disk response to a jet instability?
• Thermal X-ray emission from a baryonic jet: a self-consistent multicolour spectral model
• A re-establishing jet during an X-ray re-brightening of the Be/X-ray binary Swift J0243.6+6124
• Polarized synchrotron emission in quiescent black hole X-ray transients
• Structure of a collisionless pair jet in a magnetized electron-proton plasma: flow-aligned magnetic field
• Relativistic Tidal Acceleration of Astrophysical Jets
• Hard-X-ray-selected Active Galactic Nuclei -- II. Spectral Energy Distributions in the 5-45 GHz domain
• An upper limit on nickel overabundance in the supercritical accretion disk wind of SS 433 from X-ray spectroscopy
• Multiwavelength observations of MAXI J1820+070 during its outburst decay and subsequent mini-outburst
• Diagnostics of Parameters for the X-ray Jets of SS 433 from High-Resolution Chandra Spectroscopy
• Numerical simulations of MHD jets from Keplerian accretion disks I-Recollimation shocks
• Accretion in active galactic nuclei and disk-jet coupling
• Whispering in the dark: Faint X-ray emission from black holes with OB star companions
• A broadband radio view of transient jet ejecta in the black hole candidate X-ray binary MAXI J1535-571
• Radio/X-ray Correlation in the Mini-Outburts of Black Hole X-ray Transient GRS 1739--278
• Faint $\gamma$-ray sources at low-redshift: the radio galaxy IC 1531
• A New Microquasar Candidate in M83
• Anisotropic Gravitational Collapse and Cosmic Jets
• Advective accretion flow properties around rotating black holes - application to GRO J1655-40
• The energy distribution of electrons in radio jets
• Fourier time lags in the dwarf nova SS Cygni
• A Dependable Distance Estimator to Black Hole Low-Mass X-ray Binaries
• Accretion Disc Evolution in GRO J1655-40 and LMC X-3 with Relativistic and Non-Relativistic Disc Models
• Polarimetry of binary systems: polars, magnetic CVs, XRBs
• Evidence of mutually exclusive outflow forms from a black hole X-ray binary
• Probing AGN jet precession with LISA
• Collisionless tangential discontinuity between pair plasma and electron-proton plasma
• The Origin of Radio Emission in Black Hole X-ray Binaries
• Black hole outflows initiated by a large-scale magnetic field
• A Multi-wavelength Characterization of the 2023 Outburst of MAXI J1807+132: Manifestations of Disk Instability and Jet Emission
• A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
• Tracking optical variability and outflows across the accretion states of the black hole transient MAXI J1820+070
• On the infrared coincidence: what is the jet contribution to the X-ray power law in GX 339-4?
• Reprocessing from highly ionized gas in the soft spectral state of V4641 Sgr with NuSTAR
• Explaining the 'outliers' track in Black Hole X-ray Binaries with the BZ-jet and inner-disk coupling
• Proper Motion and Natal Kick in the Galactic Black Hole X-ray Binary AT2019wey
• X-ray and Gamma-ray Emission from a High-Temperature Plasma and the Spectra of Accreting Black Holes
• Rapid far-infrared spectral timing of X-ray binaries with PRIMA