Sources of Relativistic Jets in the Galaxy

Abstract

Black holes of stellar mass and neutron stars in binary systems are first detected as hard X-ray sources using high-energy space telescopes. Relativistic jets in some of these compact sources are found by means of multiwavelength observations with ground-based telescopes. The X-ray emission probes the inner accretion disk and immediate surroundings of the compact object, whereas the synchrotron emission from the jets is observed in the radio and infrared bands, and in the future could be detected at even shorter wavelengths. Black-hole X-ray binaries with relativistic jets mimic, on a much smaller scale, many of the phenomena seen in quasars and are thus called microquasars. Because of their proximity, their study opens the way for a better understanding of the relativistic jets seen elsewhere in the Universe. From the observation of two-sided moving jets it is inferred that the ejecta in microquasars move with relativistic speeds similar to those believed to be present in quasars. The simultaneous multiwavelength approach to microquasars reveals in short timescales the close connection between instabilities in the accretion disk seen in the X-rays, and the ejection of relativistic clouds of plasma observed as synchrotron emission at longer wavelengths. Besides contributing to a deeper comprehension of accretion disks and jets, microquasars may serve in the future to determine the distances of jet sources using constraints from special relativity, and the spin of black holes using general relativity.

39 pages, Tex, 8 figures, to appear in vol. 37 (1999) of Annual Reviews of Astronomy and Astrophysics

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• A newly discovered double-double candidate microquasar in NGC 300
• Optical Spectroscopic Observations of Cyg X-1=HDE 226868
• Microquasars as heating sources of the intergalactic medium during reionisation of the Universe
• Force-feeding Black Holes
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• Energy Extraction from Spinning Black Holes via Relativistic Jets
• V4641 Sgr: a candidate precessing microblazar
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• Double-peak spectral energy density of GRBs and the true identity of GRB 031203
• Delayed Flashes from Counter Jets of Gamma Ray Bursts
• Correlated radio:X-ray emission in the hard states of Galactic microquasars
• Radiative Hydromagnetic Shocks in Relativistic Outflow Sources
• Relativistic Outflows from Advection-Dominated Accretion Disks around Black Holes
• Kerr-Taub-NUT spacetime to explain the jet power and the radiative efficiency of astrophysical black holes
• Kink Instability of Force-Free Jets: a Parameter Space Study
• The cepheid-like relationship between variability and luminosity explained within the ``cannonball model'' of Gamma-Ray bursts
• Two Mathematically Equivalent Versions of Maxwell's Equations
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• Observations of Rapid Disk-Jet Interaction in the Microquasar GRS 1915+105
• Stochastic variability in X-ray emission from the black hole binary GRS 1915+105
• Mid-Infrared observations of GRS 1915+105 during plateau and flaring states
• Velocity Structure and Variability of [O III] Emission in Black Hole Host Globular Cluster RZ2109
• Theoretical overview on high-energy emission in microquasars
• Revisiting LS I +61 303 with VLBI astrometry
• Viscous accretion of a polytropic self-gravitating disk in the presence of wind
• Off-axis emission from relativistic plasma flows
• Very high energy gamma-rays from Centaurus X-3: indications and implications
• Evidence for periodic accretion-ejection in LSI+61303
• Origin of Multi-band Emission from the Microquasar Cygnus X--1
• Low Frequency Coherence Break in The Soft X-ray State of GRS 1915+105
• Cosmic reionization by primordial cosmic rays
• Circularly polarised radio emission from GRS 1915+105 and other X-ray binaries
• X-ray Observation of SS 433 with RXTE
• The Spectrum of SS 433 in the H and K Bands
• Estimation of the neutrino flux and resulting constraints on hadronic emission models for Cyg X-3 using AGILE data
• A Search for Very Active Stars in the Galaxy
• Galactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide
• Optical and near-infrared spectroscopy of the black hole transient 4U 1543-47 during its 2021 ultra-luminous state
• Possible contribution of X-ray binary jets to the Galactic cosmic ray and neutrino flux
• Simulations of neutrino and gamma-ray production from relativistic black-hole microquasar jets
• A model for microquasars of Population III
• Accreting Black Holes
• Tentative evidence of spatially extended GeV emission from SS433/W50
• Gamma-ray observations of MAXI J1820+070 during the 2018 outburst
• Equilibrium configuration of perfect fluid orbiting around black holes in some classes of alternative gravity theories
• Exploring the supernova remnant G308.4-1.4
• Radio QPO in the $\gamma$-ray-loud X-ray binary LS I +61${}^{\circ }$303
• A universal scaling law of black hole activity including gamma-ray bursts
• Scaling of the Anomalous Boost in Relativistic Jet Boundary Layer
• Dynamical and radiative simulations of $\gamma$-ray jets in microquasars
• Ion-dominated plasma and the origin of jets in quasars
• Identification of the optical and near-infrared counterpart of GRS 1758-258
• Structure and Magnetic Fields in the Precessing Jet System SS433 III. Evolution of the Intrinsic Brightness of the Jets from a Deep Multi-Epoch VLA Campaign
• Lattice Boltzmann model for resistive relativistic magnetohydrodynamics
• Gamma-ray binaries
• On the structure of the burst and afterglow of Gamma-Ray Bursts I: the radial approximation
• The radio flaring behaviour of GRO J1655-40: an analogy with extragalactic radio sources?
• Faint $\gamma$-ray sources at low-redshift: the radio galaxy IC 1531
• Radio emission and jets from microquasars
• INTEGRAL serendipitous detection of the gamma-ray microquasar LS 5039
• The Science Case for Simultaneous mm-Wavelength Receivers in Radio Astronomy
• Chaotic magnetic disconnections trigger flux eruptions in accretion flows channeled onto magnetically saturated Kerr black holes
• EVN and MERLIN observations of microquasar candidates at low galactic latitudes
• Electromagnetic Fields in Jets
• A microquasar model applied to unidentified gamma-ray sources
• Spectrum of jet emitting disc: Application to microquasar XTE J1118+480
• Instrumentation and Future Missions in the Upcoming Era of X-Ray Polarimetry
• Faint arc-minute extended radio emission around Cygnus X-3
• Suzaku Observations of the Galactic Center Microquasar 1E 1740.7-2942
• Time-dependent radio emission from evolving jets
• Structure and Magnetic Fields in the Precessing Jet System SS 433 II. Intrinsic Brightness of the Jets
• The Planck On-Flight Forecaster (POFF)
• Microquasars: summary and outlook
• The Simultaneous Medicina-Planck Experiment (SiMPlE): data acquisition, reduction and first results
• Radio emission of the Galactic X-rays binaries with relativistic jets
• Fireball and cannonball models of gamma ray bursts confront observations
• Numerical Relativistic Hydrodynamics Based on the Total Variation Diminishing Scheme
• On the Steady Nature of Line-Driven Disk Winds: Application to Cataclysmic Variables
• X-ray spectral cut-off and the lack of hard X-ray emission from two ultraluminous X-ray sources M81 X-6 and Holmberg IX X-1
• Electromagnetic Pulse Scattering by a Spacecraft Nearing Light Speed
• Simultaneous long-term monitoring of LS I +61°303 by OVRO and Fermi-LAT
• The radio jets of SS 433 at millimetre wavelengths
• The energy distribution of electrons in radio jets
• Is J 133658.3-295105 a Radio Source at z >= 1.0 or at the Distance of M 83?
• Gamma-ray bursts and other sources of giant lightning discharges in protoplanetary systems
• A method of incorporating general relativity in electromagnetic particle-in-cell code
• The Cosmic-Ray Spectra: News on their Knees
• On the X-ray lines in the afterglows of GRBs
• A model of rotating hotspots for 3:2 frequency ratio of HFQPOs in black hole X-ray binaries
• Identification of a 12-17 day timescale in X-ray observations of GRS 1915+105
• Lithium synthesis in microquasar accretion
• Gamma-ray binaries beyond one-zone models: an application to LS 5039
• Viscous boundary layers of radiation-dominated, relativistic jets. I. The two-stream model
• Roles of the kinetic and dynamic mechanisms in the $L_p-E_p$ relation
• Black holes at cosmic dawn in the redshifted 21cm signal of HI
• High Energy Gamma Rays from Nebulae Associated with Extragalactic Microquasars and Ultra-Luminous X-ray Sources
• HST/NICMOS Observations of Fast Infrared Flickering in the Microquasar GRS 1915+105
• Formation of Sco X-1 induced by anomalous magnetic braking of Ap/Bp stars
• Spectropolarimetric Study on Circumstellar Structure of Microquasar LS I +61deg 303
• Quenched millimetre emission from Cygnus X-1 in a soft X-ray state
• High-energy gamma-ray Emission from Microquasars: LS 5039 and LS I +61 303
• Neutrinos from microquasars
• Relativistic Magnetized Astrophysical Plasma Outflows in Black-Hole Microquasars
• Correlation between 3:2 QPO pairs and Jets in Black Hole X-ray Binaries
• Hour time-scale QPOs in the X-ray and radio emission of LS I +61${}^{\circ }$303
• Impact of ionization and electron density gradients in X-ray reflection spectroscopy measurements
• X-ray triple rings around the M87 jets in the central Virgo cluster
• IR spectra of the microquasar GRS 1915+105 during a low state
• Radio spectra of protostellar jets: Thermal and non-thermal emission
• The radio surroundings of the microquasar GRO J1655-40
• AGNs and microquasars as high energy gamma-ray sources
• Particle acceleration in astrophysical shear flows
• Owens Valley Radio Observatory monitoring of LS I +61°303 completes three cycles of the super-orbital modulation
• Flares In Long And Short Gamma Ray Bursts
• Relativistic stellar jets: dynamics and non-thermal radiation
• Hot Settling Accretion Flow onto a Spinning Black Hole
• Theoretical thermal X-ray spectra of relativistic MHD jets
• Extending the "Energetic Scaling of Relativistic Jets From Black Hole Systems" to Include $\gamma$-ray-loud X-ray Binaries
• Exploring the role of composition and mass-loading on the properties of hadronic jets
• Approaching the black hole by numerical simulations
• Accretion disc winds in X-ray binaries
• A year-long AGILE observation of Cygnus X-1 in hard spectral state
• An accretion model for the growth of the central black hole associated with ionization instability in quasars
• Multiwavelength modeling the SED of Luminous Supersoft X-ray Sources in Large Magellanic Cloud and Small Magellanic Cloud
• Black Hole High Mass X-ray Binary Microquasars at Cosmic Dawn
• Variation of the gas and radiation content in the sub-Keplerian accretion disk around black holes and its impact to the solutions
• A new search strategy for microquasar candidates using NVSS/2MASS and XMM-Newton data
• VHE Gamma-rays from Galactic X-ray Binary Systems
• Large-scale radio bubbles around the black hole transient V4641 Sgr
• A Unified Model of High-Energy Astrophysical phenomena
• Observed jet power and radiative efficiency of black hole candidates in Kerr + PFDM model
• The effect of dissipative corona on the structure and stability of cold optically thick accretion disks at high accretion rates
• Towards a population of HMXB/NS microquasars as counterparts of low-latitude unidentified EGRET sources
• Modeling of thermal and non-thermal radio emission from HH80-81 jet
• Relativistic-Amplitude electromagnetic waves - Beating the "magnetic" barrier
• Ultra Fast Self-Compton Cooling
• Detection of the microquasar V404 Cygni at gamma-rays revisited: short flaring events in quiescence
• Black Hole Spectral States and Physical Connections
• Extended Radio Structures and a Compact X-ray Cool-Core in the Cluster Source PKS 1353-341
• Radio/X-ray correlations and variability in the X-ray binary LS I +61°303
• Steady jet ejections from the innermost region of advection-dominated accretion flow around a black hole
• Impact of temperature asymmetry and small fraction of static positive ions on the relaxed states of a relativistic hot pair plasma
• Synthetic Neutrino Imaging of a Microquasar
• Effect of magnetic field inclination on black hole jet power and particle acceleration
• Hydrodynamical winds from two-temperature plasma in X-ray binaries
• HAWC Search for High-Mass Microquasars
• Results from MAGIC's first observation cycle on galactic sources
• On the binary nature of 1RXS J162848.1-415241
• A solution of a hoary conundrum: the origin and properties of cosmic rays
• An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105
• Universal Peaks Ratio In The Spectral Energy Density Of Double Hump Blazars, Gamma Ray Bursts, And Microquasars
• New evidence on the origin of the microquasar GRO J1655-40
• The Non-thermal Radio Jet Toward the NGC 2264 Star Formation Region
• Synchrotron emission from secondary leptons in microquasar jets
• Simulated Radio and Neutrino Imaging of a Microquasar
• Transient jet ejections associated with limit-cycle behaviors in the very high state of black hole binaries
• Optical/IR counterpart to the resolved X-ray jet source CXO J172337.5-373442 and its distance
• Neutrino Emission from Proton Photon Jet Interactions in Microquasars
• Stellar black holes: cosmic history and feedback at the dawn of the universe
• The Cygnus X region XXIII. Is 18P87 galactic or extragalactic?
• Intranight optical monitoring of the rare quasar J0950+5128, the brightest known candidate for transition from radio-quiet to radio-loud state
• Microquasars: disk-jet coupling in stellar-mass black holes
• Shock corrugation to the rescue of the internal shock model in microquasars: The single-scale MHD view
• Jets from compact objects
• A two-step strategy to identify episodic sources of gravitational waves and high energy neutrinos in starburst galaxies
• Proper Motion and Natal Kick in the Galactic Black Hole X-ray Binary AT2019wey
• Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433
• Microquasar models for 3EG J1828+0142 and 3EG J1735-1500
• Non-Thermal Emission from Galactic Jets
• Constraints Preserving Lax-Wendroff Flux Reconstruction for Relativistic Hydrodynamics with General Equations of State
• Effects of radiative losses on the relativistic jets of high-mass microquasars
• X-ray and Gamma-ray Emission from a High-Temperature Plasma and the Spectra of Accreting Black Holes
• High Velocity HI Jet-like Feature Towards the SNR Candidate G351.7-1.2
• Synergies in extragalactic and Galactic jet research
• Relativistic hydrodynamical simulations of the effects of the stellar wind and the orbit on high-mass microquasar jets
• Long time-scale variability of X-ray binaries with late type giant companions