The dynamical structure of the outflows driven by a large-scale magnetic field
arXiv:2111.15115 · doi:10.3847/1538-4357/ac3df4
Abstract
Large-scale magnetic field is crucial in launching and collimating the jets/outflows. It is found that the magnetic flux can be efficiently transported inward by the fast moving corona above a thin disk. In this work we investigate the dynamical structure of the outflows driven by the large-scale magnetic field advected by the hot corona. With derived large-scale magnetic field, the outflow solution along every field line is obtained by solving a set of magneto-hydrodynamical (MHD) Equations self-consistently with boundary conditions at the upper surface of the corona. We find that the terminal speeds of the outflows driven from the inner region of the disk are . The temperatures of the outflows at the large distance from the black hole are still as high as several ten keV. The properties of the magnetic outflows derived in this work are roughly consistent with the fast outflows detected in some luminous quasars and X-ray binaries. The total mass loss rate in the outflows from the corona is about of the mass accretion rate of the disk. The three dimension field geometry, the velocity, temperature and density of the outflows derived in this work can be used for calculating the emergent spectra and their polarization of the accretion disk/corona/outflow systems. Our results may help understand the features of the observed spectra of X-ray binaries and active galactic nuclei.
arXiv commentaccepted for publication in ApJ
References in corpus (93)
- Observational Evidence of AGN Feedback
- Towards a unified model for black hole X-ray binary jets
- Heating Hot Atmospheres with Active Galactic Nuclei
- Dynamics of line-driven disk winds in Active Galactic Nuclei
- Black holes in galaxy mergers: The formation of red elliptical galaxies
- First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon
- Evidence for ultra-fast outflows in radio-quiet AGNs: I - detection and statistical incidence of Fe K-shell absorption lines
- Dynamics of Line-Driven Disk Winds in Active Galactic Nuclei II: Effects of Disk Radiation
- Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows
- Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy
- Plasma Ejection from Magnetic Flares and the X-ray Spectrum of Cygnus X-1
- Unification of X-ray winds in Seyfert galaxies: from ultra-fast outflows to warm absorbers
- The magnetic nature of disk accretion onto black holes
- Local Study of Accretion Disks with a Strong Vertical Magnetic Field: Magnetorotational Instability and Disk Outflow
- MHD simulations of jet acceleration from Keplerian accretion disks: the effects of disk resistivity
- The Accretion Disk Wind in the Black Hole GRO J1655-40
- A Compton-thick Wind in the High Luminosity Quasar, PDS 456
- Coronal outflow dominated accretion discs: a new possibility for low luminosity black holes?
- Magneto-thermal Disk Wind from Protoplanetary Disks
- MHD Accretion-Disk Winds as X-ray Absorbers in AGNs
- Magnetized Accretion-Ejection Structures: 2.5D MHD simulations of continuous Ideal Jet launching from resistive accretion disks
- Large-Scale Poloidal Magnetic Field Dynamo Leads to Powerful Jets in GRMHD Simulations of Black Hole Accretion with Toroidal Field
- Transport of Large Scale Poloidal Flux in Black Hole Accretion
- Global Evolution of an Accretion Disk with Net Vertical Field: Coronal Accretion, Flux Transport, and Disk Winds
- Magnetic reconnection: flares and coronal heating in Active Galactic Nuclei
- A unified accretion-ejection paradigm for Black Hole X-ray Binaries
- Discovery of ultra-fast outflows in a sample of Broad Line Radio Galaxies observed with Suzaku
- Cosmic evolution of stellar quenching by AGN feedback: clues from the Horizon-AGN simulation
- The hard X-ray spectral evolution in X-ray binaries and its application to constrain the black hole mass of ultraluminous X-ray sources
- MHD Simulations of Global Accretion Disks with Vertical Magnetic Fields
- Magnetic flux captured by an accretion disk
- Evidence for a Variable Ultrafast Outflow in the Newly Discovered Ultraluminous Pulsar NGC 300 ULX-1
- Line-driven Disk Winds in Active Galactic Nuclei: The Critical Importance of Ionization and Radiative Transfer
- The Turbulent Magnetic Prandtl Number of MHD Turbulence in Disks
- The Fragmentation of Pre-enriched Primordial Objects
- Radiatively inefficient MHD accretion-ejection structures
- Two-temperature coronal flow above a thin disk
- Turbulent resistivity driven by the magnetorotational instability
- Transport of magnetic flux and the vertical structure of accretion discs: I. Uniform diffusion coefficients
- An accretion disc-corona model for X-ray spectra of active galactic nuclei
- Magnetically-Driven Accretion-Disk Winds and Ultra-Fast Outflows in PG1211+143
- Magnetic flares in accretion disc coronae and the Spectral States of black hole candidates: the case of GX 339-4
- Strongly magnetized accretion disks: structure and accretion from global magnetohydrodynamic simulations
- The Disk Wind in the Rapidly Spinning Stellar-Mass Black Hole 4U 1630-472 Observed with NuSTAR
- Advection/Diffusion of Large-Scale B-Field in Accretion Disks
- The large scale magnetic fields of thin accretion disks
- Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070
- Bipolar jets launched from magnetically diffusive accretion disks. I. Ejection efficiency vs field strength and diffusivity
- The origin of ultra-fast outflows in AGN: Monte-Carlo simulations of the wind in PDS 456
- Transport of magnetic flux and the vertical structure of accretion discs: II. Vertical profile of the diffusion coefficients
- Are X-ray Emitting Coronae around Super Massive Black Holes Outflowing?
- The Disk-Wind-Jet Connection in the Black Hole H 1743-322
- Revealing the ultra-fast outflow in IRAS 13224-3809 through spectral variability
- On the Observational Difference Between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei
- The Intrinsic Far-infrared Continua of Type-1 Quasars
- Variation of ionizing continuum: the main driver of Broad Absorption Line Variability
- Resolving the soft X-ray ultra fast outflow in PDS 456
- An Obscured, Seyfert-2-like State of the Stellar-mass Black Hole GRS 1915+105 Caused by Failed Disk Winds
- Analytical Solution of Magnetically Dominated Astrophysical Jets and Winds: Jet Launching, Acceleration, and Collimation
- The properties of broad absorption line outflows based on a large sample of quasars
- Modelling MHD accretion-ejection - episodic ejections of jets triggered by a mean-field disk dynamo
- The outflows accelerated by the magnetic fields and radiation force of accretion disks
- Thermal stability of thin disk with magnetically driven winds
- X-ray evidence for the accretion disc-outflow connection in 3C 111
- A general relativistic model of accretion disks with coronae surrounding Kerr black holes
- An extensive numerical survey of the correlation between outflow dynamics and accretion disk magnetization
- Variable Nature of Magnetically-Driven Ultra-Fast Outflows
- Physical Conditions in Ultra Fast Outflows in AGN
- Testing the disk-corona interplay in radiatively-efficient broad-line AGN
- The large-scale magnetic field of a thin accretion disk with outflows
- Fast Inflow Directly Feeding Black Hole Accretion Disk in Quasars
- Magnetized Disk-Winds in NGC 3783
- A variable ionized disk wind in the black-hole candidate EXO 1846-031
- Wobbling and precessing jets from warped disks in binary systems
- Testing wind as an explanation for the spin problem in the continuum-fitting method
- The high efficiency jets magnetically accelerated from a thin disk in powerful lobe-dominated FRII radio galaxies
- Long-term simulation of MHD jet launching from an orbiting star-disk system
- Magnetic-reconnection-heated corona in active galactic nuclei: refined disc-corona model and application to broad-band radiation
- A systematic study of the condensation of the corona and the application for correlation in luminous active galactic nuclei
- X-ray properties of dust-obscured galaxies with broad optical/UV emission lines
- Revisiting the structure and spectrum of the magnetic-reconnection-heated corona in luminous AGNs
- The power of the jets accelerated by the coronal magnetic field
- Insight-HXMT observations of a possible fast transition from jet to wind dominated state during a huge flare of GRS~1915+105
- Numerical simulations of winds driven by radiation force from the corona above a thin disk
- Jets in the soft state in Cyg X-3 caused by advection of the donor magnetic field and unification with low-mass X-ray binaries
- Magnetohydrodynamic Winds Driven by the Line Force from the Standard Thin Disk around Supermassive Black Holes. I. The Case of Weak Magnetic Field
- Magnetic field transport in compact binaries
- Jet production in black-hole X-ray binaries and active galactic nuclei: mass feeding and advection of magnetic fields
- Magnetohydrodynamic winds driven by line force from the standard thin disk around supermassive black holes: II. a possible model for ultra-fast outflows in radio-loud AGNs
- The large-scale magnetic field advected in the corona of a thin accretion disk
- Thermal wind from hot accretion flows at large radii
- Magnetohydrodynamic numerical simulation of the outflows driven by magnetic field and radiation force from the corona above a thin disk
- An extreme Ultraluminous X-ray source X-1 in NGC 5055