On the wind production from hot accretion flows with different accretion rates
arXiv:1711.02238 · doi:10.1093/mnras/stx2894
Abstract
We perform two-dimensional simulations to study how the wind strength changes with accretion rate. We take into account bremsstrahlung, synchrotron radiation and the Comptonization. We find that when the accretion rate is low, radiative cooling is not important, the accretion flow is hot accretion flow. For the hot accretion flow, wind is very strong. The mass flux of wind can be of the mass inflow rate. When the accretion rate increases to a value at which radiative cooling rate is roughly equal to or slightly larger than viscous heating rate, cold clumps can form around the equatorial plane. In this case, the gas pressure gradient force is small and wind is very weak. Our results may be useful for the sub-grid model of active galactic nuclear feedback study.
arXiv comment9 pages, 8 figures, accepted by MNRAS
References in corpus (80)
- X-ray Properties of Black-Hole Binaries
- Advection-Dominated Accretion: A Self-Similar Solution
- Modeling feedback from stars and black holes in galaxy mergers
- Advection-Dominated Accretion: Underfed Black Holes and Neutron Stars
- Hot Accretion Flows Around Black Holes
- Towards a unified model for black hole X-ray binary jets
- Advection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991
- Efficient Generation of Jets from Magnetically Arrested Accretion on a Rapidly Spinning Black Hole
- Nuclear Activity in Nearby Galaxies
- General Relativistic Magnetohydrodynamic Simulations of Magnetically Choked Accretion Flows around Black Holes
- Dynamics of line-driven disk winds in Active Galactic Nuclei
- Nonthermal Electrons in Radiatively Inefficient Accretion Flow Models of Sagittarius A*
- Powerful Outflows and Feedback from Active Galactic Nuclei
- Thermal Equilibria of Accretion Disks
- Three-dimensional MHD Simulations of Radiatively Inefficient Accretion Flows
- GRMHD Simulations of Magnetized Advection Dominated Accretion on a Non-Spinning Black Hole: Role of Outflows
- Advection-Dominated Accretion and the Black Hole Event Horizon
- Hydrodynamical Non-radiative Accretion Flows in Two-Dimensions
- Radiative feedback from massive black holes in elliptical galaxies. AGN flaring and central starburst fueled by recycled gas
- Cooling flows and quasars: II. Detailed models of feedback modulated accretion flows
- Magnetically Driven Accretion Flows in the Kerr Metric I: Models and Overall Structure
- States and transitions in black-hole binaries
- A New Simple Model for High Frequency Quasi Periodic Oscillations in Black Hole Candidates
- Radiative Processes, Spectral States and Variability of Black-Hole Binaries
- The Dynamical Structure of Nonradiative Black Hole Accretion Flows
- Cooling flows and quasars: different aspects of the same phenomenon? I. Concepts
- The Influence of Magnetic Field Geometry on the Evolution of Black Hole Accretion Flows: Similar Disks, Drastically Different Jets
- Numerical Simulation of Hot Accretion Flows (II): Nature, Origin, and Properties of Outflow and Their Possible Observational Applications
- Feedback from Central Black Holes in Elliptical Galaxies: Two-dimensional Models Compared to One-dimensional Models
- Local Study of Accretion Disks with a Strong Vertical Magnetic Field: Magnetorotational Instability and Disk Outflow
- Spectral Models of Advection-Dominated Accretion Flows with Winds
- Magnetohydrodynamical Non-radiative Accretion Flows in Two-Dimensions
- Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
- Numerical Simulation of Hot Accretion Flows (I): A Large Radial Dynamical Range and the Density Profile of Accretion Flow
- Prograde and Retrograde Black Holes: Whose Jet is More Powerful?
- Suppressing star formation in quiescent galaxies with supermassive black hole winds
- Energy, momentum and mass outflows and feedback from thick accretion discs around rotating black holes
- Two-dimensional models of hydrodynamical accretion flows into black holes
- Feedback from Mass Outflows in Nearby Active Galactic Nuclei I. UV and X-ray Absorbers
- Oscillations of vertically integrated relativistic tori -- I. Axisymmetric modes in a Schwarzschild spacetime
- Ultra-fast outflows in radio-loud active galactic nuclei
- A Magnetohydrodynamic Nonradiative Accretion Flow in Three Dimensions
- Discovery of ultra-fast outflows in a sample of Broad Line Radio Galaxies observed with Suzaku
- Observational appearance of inefficient accretion flows and jets in 3D GRMHD simulations: Application to Sgr~A*
- Radiatively Inefficient Accretion: Breezes, Winds and Hyperaccretion
- Global Simulations of Accretion Disks I: Convergence and Comparisons with Local Models
- Radiative, two-temperature simulations of low luminosity black hole accretion flows in general relativity
- Quasi-periodic accretion and gravitational waves from oscillating "toroidal neutron stars" around a Schwarzschild black hole
- Dynamics of Accretion Flows Irradiated by a Quasar
- Luminous hot accretion disks
- Rotating Accretion Flows: From Infinity to the Black Hole
- Low-Luminosity Accretion in Black Hole X-ray Binaries and Active Galactic Nuclei
- Dynamics of oscillating relativistic tori around Kerr black holes
- Locality of MHD Turbulence in Isothermal Disks
- Oscillation modes of relativistic slender tori
- The large scale magnetic fields of advection dominated accretion flows
- Evidence for simultaneous jets and disk winds in luminous low-mass X-ray binaries
- The Shakura-Sunyaev Viscosity Prescription with Variable alpha(r)
- The Fate of Non-Radiative Magnetized Accretion Flows: Magnetically-Frustrated Convection
- The Effect of the AGN Feedback on the Interstellar Medium of Early-Type Galaxies: 2D Hydrodynamical Simulations of the Low-Rotation Case
- Numerical Parameter Survey of Nonradiative Black Hole Accretion -- Flow Structure and Variability of the Rotation Measure
- The Radiative Efficiency and Spectra of Slowly Accreting Black Holes from Two-Temperature GRRMHD Simulations
- Empirical relation between angular momentum transport and thermal-to-magnetic pressure ratio in shearing box simulations
- Luminous hot accretion flows: thermal equilibrium curve and thermal stability
- Mechanism of Outflows in Accretion System: Advective Cooling Cannot Balance Viscous Heating?
- Hydrodynamical numerical simulation of wind production from black hole hot accretion flows at very large radii
- On the large-scale outflows in active galactic nuclei: consequences of coupling the mass-supply rate and accretion luminosity
- AGN feedback in an isolated elliptical galaxy: the effect of strong radiative feedback in the kinetic mode
- On the convective instability of hot radiative accretion flows
- A Physical Link Between Jet Formation and Hot Plasma in Active Galactic Nuclei
- Magneto-hydrodynamical Numerical simulation of wind production from black hole hot accretion flows at very large radii
- Thermal stability of thin disk with magnetically driven winds
- Global Compton heating and cooling in hot accretion flows
- Hot accretion flow with radiative cooling: state transitions in black hole X-ray binaries
- Quasi-periodic oscillations from relativistic hydrodynamical slender tori
- Monte Carlo simulations of global Compton cooling in inner regions of hot accretion flows
- Two-dimensional inflow-wind solution of black hole accretion with an evenly symmetric magnetic field
- Three-dimensional magnetohydrodynamical simulations of the morphology of head-tail radio galaxies based on magnetic tower jet model
- Compton Heated Outflow from CDAFs
- Acceleration of wind in optically thin and thick black hole accretion disks simulated in general relativity
Cited by in corpus (14)
- Radiative Properties of Magnetically-Arrested Disks
- The Origin of Matter at the Base of Relativistic Jets in Active Galactic Nuclei
- The self-similar structure of advection-dominated discs with outflow and radial viscosity
- Thermal Equilibrium Solutions of Black Hole Accretion Flows: Outflows VS Advection
- Winds and feedback from supermassive black holes accreting at low rates: Hydrodynamical treatment
- Large-scale Dynamics of Winds Driven by Line Force from a Thin Accretion Disk
- Hot accretion flow around neutron stars
- Self-similar structure of resistive ADAFs with outflow and large-scale magnetic field
- Two-temperature radiative hot accretion flow around neutron stars
- Black holes: accretion processes in X-ray binaries
- The width-flux relation of the broad iron line during the state transition of the black hole X-ray binaries
- Self-similar Solution of Hot Accretion Flow with Thermal Conduction and Anisotropic Pressure
- Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius
- Thermal Conduction in Clumpy Disks and BLR clouds