Radiation-driven outflows in AGNs: Revisiting feedback effects of scattered and reprocessed photons
arXiv:1910.00288 · doi:10.1093/mnras/stz2758
Abstract
We perform two-dimensional hydrodynamical simulations of slowly rotating accretion flows in the region of around a supermassive black holes with . The accretion flow is irradiated by the photons from the central active galactic nucleus (AGN). In addition to the direct radiation from the AGN, we have also included the "re-radiation", i.e., the locally produced radiation by Thomson scattering, line and bremsstrahlung radiation. Compare to our previous work, we have improved the calculation of radiation force due to the Thomson scattering of X-ray photons from the central AGN. We find that this improvement can significantly increase the mass flux and velocity of outflow. We have compared the properties of outflow --- including mass outflow rate, velocity, and kinetic luminosity of outflow --- in our simulation with the observed properties of outflow in AGNs and found that they are in good consistency. This implies that the combination of line and re-radiation forces is the possible origin of observed outflow in luminous AGNs.
arXiv comment14 pages, 6 figures; accepted for publication in MNRAS
References in corpus (50)
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- The Demography of Massive Dark Objects in Galaxy Centres
- A Relationship Between Nuclear Black Hole Mass and Galaxy Velocity Dispersion
- Observational Evidence of AGN Feedback
- The slope of the black-hole mass versus velocity dispersion correlation
- The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
- On the Black Hole Mass - Bulge Mass Relation
- The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
- On the Fate of Gas Accreting at a Low Rate onto a Black Hole
- Simulating galaxy formation with black hole driven thermal and kinetic feedback
- Dynamics of line-driven disk winds in Active Galactic Nuclei
- Evidence for ultra-fast outflows in radio-quiet AGNs: I - detection and statistical incidence of Fe K-shell absorption lines
- GRMHD Simulations of Magnetized Advection Dominated Accretion on a Non-Spinning Black Hole: Role of Outflows
- Super-critical Accretion Flows around Black Holes: Two-dimensional, Radiation-pressure-dominated Disks with Photon-trapping
- Black Hole Masses and Eddington Ratios at 0.3<z<4
- An expanded M_bh-sigma diagram, and a new calibration of active galactic nuclei masses
- 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
- Simulating Radiating and Magnetized Flows in Multi-Dimensions with ZEUS-MP
- Dissecting X-ray-emitting Gas around the Center of our Galaxy
- Cooling flows and quasars: different aspects of the same phenomenon? I. Concepts
- Numerical Simulation of Hot Accretion Flows (II): Nature, Origin, and Properties of Outflow and Their Possible Observational Applications
- Momentum Driving: which physical processes dominate AGN feedback?
- Numerical Simulation of Hot Accretion Flows (III): Revisiting wind properties using trajectory approach
- Quasars: the characteristic spectrum and the induced radiative heating
- Numerical Simulation of Hot Accretion Flows (I): A Large Radial Dynamical Range and the Density Profile of Accretion Flow
- Evidence for ultra-fast outflows in radio-quiet AGNs: III - location and energetics
- Suppressing star formation in quiescent galaxies with supermassive black hole winds
- Ultra-fast outflows in radio-loud active galactic nuclei
- Active Galactic Nuclei Feedback in an Elliptical Galaxy with the Most Updated AGN Physics (I): Low-angular Momentum Case
- Dynamics of Accretion Flows Irradiated by a Quasar
- Rotating Accretion Flows: From Infinity to the Black Hole
- The Quasar Mass-Luminosity Plane I: A Sub-Eddington Limit for Quasars
- Multiwavelength campaign on Mrk 509 VIII. Location of the X-ray absorber
- Evidence for simultaneous jets and disk winds in luminous low-mass X-ray binaries
- Dynamics of Rotating Accretion Flows Irradiated by a Quasar
- 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
- Two dimensional numerical simulations of Supercritical Accretion Flows revisited
- The properties of broad absorption line outflows based on a large sample of quasars
- Magneto-hydrodynamical Numerical simulation of wind production from black hole hot accretion flows at very large radii
- Comparison of ejection events in the jet and accretion disc outflows in 3C 111
- Spectral Energy Distribution of the inner accretion flow around Sgr A* -- Clue for a weak outflow in the innermost region
- Active Galactic Nuclei Feedback in an Elliptical Galaxy with the Most Updated AGN Physics (II): High-Angular Momentum Case
- Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties
- Three-Dimensional Simulations of Inflows Irradiated by a Precessing Accretion Disk in Active Galactic Nuclei: Formation of Outflows
- Radiation driven outflow in active galactic nuclei: the feedback effects of scattered and reprocessed photons
- MACER improved: AGN feedback computed in rotating early-type galaxies at high resolution
- Two-dimensional inflow-wind solution of black hole accretion with an evenly symmetric magnetic field
Cited by in corpus (6)
- Ionized outflows from active galactic nuclei as the essential elements of feedback
- Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. III. Results for the Seyfert 2 Galaxies Markarian 3, Markarian 78, and NGC 1068
- The picture of BLR in 2.5-D FRADO: Dynamics & Geometry
- Two-dimensional Inflow-outflow Solution of Supercritical Accretion Flow
- The Unusual AGN Host NGC 1266: Evidence for Shocks in a Molecular Gas Rich S0 Galaxy with a Low Luminosity Nucleus
- Line Driven Winds from Variable Accretion Discs