Self-regulated AGN feedback of light jets in cool-core galaxy clusters
arXiv:2204.01765 · doi:10.1093/mnras/stac2860
Abstract
Heating from active galactic nuclei (AGN) is thought to stabilize cool-core clusters, limiting star formation and cooling flows. We employ radiative magneto-hydrodynamic (MHD) simulations to model light AGN jet feedback with different accretion modes (Bondi-Hoyle-Lyttleton and cold accretion) in an idealised Perseus-like cluster. Independent of the probed accretion model, accretion efficiency, jet density and resolution, the cluster self-regulates with central entropies and cooling times consistent with observed cool-core clusters in this non-cosmological setting. We find that increased jet efficiencies lead to more intermittent jet powers and enhanced star formation rates. Our fiducial low-density jets can easily be deflected by orbiting cold gaseous filaments, which redistributes angular momentum and leads to more extended cold gas distributions and isotropic bubble distributions. In comparison to our fiducial low momentum-density jets, high momentum-density jets heat less efficiently and enable the formation of a persistent cold-gas disc perpendicular to the jets that is centrally confined. Cavity luminosities measured from our simulations generally reflect the cooling luminosities of the intracluster medium (ICM) and correspond to averaged jet powers that are relatively insensitive to short periods of low-luminosity jet injection. Cold gas structures in our MHD simulations with low momentum-density jets generally show a variety of morphologies ranging from discy to very extended filamentary structures. In particular, magnetic fields are crucial to inhibit the formation of unrealistically massive cold gas discs by redistributing angular momentum between the hot and cold phases and by fostering the formation of elongated cold filaments that are supported by magnetic pressure.
arXiv comment26 pages, 19 figures, published in MNRS
References in corpus (116)
- The Global Schmidt Law in Star Forming Galaxies
- Observational Evidence of AGN Feedback
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- Cosmological SPH simulations: A hybrid multi-phase model for star formation
- Simulating Galaxy Formation with the IllustrisTNG Model
- A model for cosmological simulations of galaxy formation physics
- A Systematic Study of Radio-Induced X-ray Cavities in Clusters, Groups, and Galaxies
- Mechanical Feedback from Active Galactic Nuclei in Galaxies, Groups, and Clusters
- The Feedback-Regulated Growth of Black Holes and Bulges through Gas Accretion and Starbursts in Cluster Central Dominant Galaxies
- Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters
- X-ray Spectroscopy of Cooling Clusters
- What is a Cool-Core Cluster? A Detailed Analysis of the Cores of the X-ray Flux-Limited HIFLUGCS Cluster Sample
- XMM-Newton observations of the Perseus Cluster I: The temperature and surface brightness structure
- Improving the convergence properties of the moving-mesh code AREPO
- Thermal Instability in Gravitationally-Stratified Plasmas: Implications for Multi-Phase Structure in Clusters and Galaxy Halos
- Thermal Instability & the Feedback Regulation of Hot Halos in Clusters, Groups, and Galaxies
- Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets
- Simulations of magnetic fields in isolated disk galaxies
- Magnetohydrodynamics on an unstructured moving grid
- Feedback Heating by Cosmic Rays in Clusters of Galaxies
- A deeper X-ray study of the core of the Perseus galaxy cluster: the power of sound waves and the distribution of metals and cosmic rays
- Draping of Cluster Magnetic Fields over Bullets and Bubbles -- Morphology and Dynamic Effects
- An Entropy Threshold for Strong H-alpha and Radio Emission in the Cores of Galaxy Clusters
- On the Nature of Feedback Heating in Cooling Flow Clusters
- Raining on black holes and massive galaxies: the top-down multiphase condensation model
- Near Infrared Spectroscopy of High Redshift Active Galactic Nuclei. I. A Metallicity-Accretion Rate Relationship
- Cooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters
- Magnetic field formation in the Milky Way-like disk galaxies of the Auriga project
- Cold, clumpy accretion onto an active supermassive black hole
- A Mechanism for Stimulating AGN Feedback by Lifting Gas in Massive Galaxies
- How AGN Jets Heat the Intracluster Medium -- Insights from Hydrodynamic Simulations
- Chandra Observation of the Cooling Flow Cluster Abell 2052
- A uniform metal distribution in the intergalactic medium of the Perseus cluster of galaxies
- Ubiquitous cold and massive filaments in cool core clusters
- Cool core cycles: Cold gas and AGN jet feedback in cluster cores
- Inside the Bondi radius of M87
- Interaction of Radio Lobes with the Hot Intracluster Medium: Driving Convective Outflow in Hydra A
- Modeling AGN Feedback in Cool-Core Clusters: The Balance between Heating and Cooling
- The answer is blowing in the wind: Simulating the interaction of jets with dynamic cluster atmospheres
- Cooling Time, Freefall Time, and Precipitation in the Cores of ACCEPT Galaxy Clusters
- Particle content, radio-galaxy morphology and jet power: all radio-loud AGN are not equal
- Chaotic cold accretion on to black holes in rotating atmospheres
- Impact of tangled magnetic fields on AGN-blown bubbles
- An Observationally Motivated Framework for AGN Heating of Cluster Cores
- Interaction of a cold cloud with a hot wind: the regimes of cloud growth and destruction and the impact of magnetic fields
- Are Radio AGN Powered by Accretion or Black Hole Spin?
- A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole
- Driving massive molecular gas flows in central cluster galaxies with AGN feedback
- Simulations of cosmic ray feedback by AGN in galaxy clusters
- AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
- Cosmic ray feedback heating of the intracluster medium
- The nature of the molecular gas system in the core of NGC 1275
- Simulating the interaction of jets with the intra-cluster medium
- The Origin of Molecular Clouds In Central Galaxies
- Interplay among Cooling, AGN Feedback and Anisotropic Conduction in the Cool Cores of Galaxy Clusters
- ALMA observations of cold molecular gas filaments trailing rising radio bubbles in PKS0745-191
- A 40-billion solar mass black hole in the extreme core of Holm 15A, the central galaxy of Abell 85
- Simulations of the dynamics of magnetised jets and cosmic rays in galaxy clusters
- Kinematics and Excitation of the Molecular Hydrogen Accretion Disc in NGC 1275
- Toward a comprehensive model for feedback by active galactic nuclei: new insights from M87 observations by LOFAR, Fermi and H.E.S.S
- MHD Simulations of AGN Jets in a Dynamic Galaxy Cluster Medium
- Heating Cooling Flows with Weak Shock Waves
- How Big Can a Black Hole Grow?
- Constraining the Nature of X-ray Cavities in Clusters and Galaxies
- Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
- AGN Heating in Simulated Cool-Core Clusters
- Magnetising the circumgalactic medium of disk galaxies
- Swimming against the current: Simulations of central AGN evolution in dynamic galaxy clusters
- Thermodynamic properties, multiphase gas and AGN feedback in a large sample of giant ellipticals
- Close entrainment of massive molecular gas flows by radio bubbles in the central galaxy of Abell 1795
- The Cosmological Impact of Luminous TeV Blazars III: Implications for Galaxy Clusters and the Formation of Dwarf Galaxies
- The particle content of low-power radio galaxies in groups and clusters
- Faraday rotation maps of disk galaxies
- Faraday Rotation Observations of Magnetic Fields in galaxy Clusters
- Blandford-Znajek jets in galaxy formation simulations: method and implementation
- Triggering and Delivery Algorithms for AGN Feedback
- Cosmic ray heating in cool core clusters - II. Self-regulation cycle and non-thermal emission
- Multiphase gas in the circumgalactic medium: relative role of and density fluctuations
- Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback
- Revealing the velocity structure of the filamentary nebula in NGC 1275 in its entirety
- Simulations of Jet Heating in Galaxy Clusters: Successes and Challenges
- Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster
- Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far infrared-radio correlation
- Cool-Core Clusters : Role of BCG, Star Formation & AGN-Driven Turbulence
- Highly ordered magnetic fields in the tail of the jellyfish galaxy JO206
- A Powerful AGN Outburst in RBS 797
- Unveiling the composition of radio plasma bubbles in galaxy clusters with the Sunyaev-Zel'dovich effect
- Constraints on the Thermal Contents of the X-ray Cavities of Cluster MS 0735.6+7421 with Sunyaev-Zel'dovich Effect Observations
- AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
- Turbulent density and pressure fluctuations in the stratified intracluster medium
- Star Formation Activity in CLASH Brightest Cluster Galaxies
- Bubble-Wrap for Bullets: The Stability Imparted By A Thin Magnetic Layer
- Do jets precess... or even move at all?
- AGN Feedback and Multi-phase Gas in Giant Elliptical Galaxies
- Quantification of Uncertainty in the Measurement of Magnetic Fields in Clusters of Galaxies
- Non-Kolmogorov turbulence in multiphase intracluster medium driven by cold gas precipitation and AGN jets
- Fountains and storms: The role of AGN and mergers in disrupting the cool-core in the RomulusC simulation
- Inflating Fat Bubbles in Clusters of Galaxies by Precessing Massive Slow Jets
- The imprints of AGN feedback within a supermassive black hole's sphere of influence
- The Presence of Thermally Unstable X-ray Filaments and the Production of Cold Gas in the NGC 5044 Group
- AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
- Bubble-driven Gas Uplift in Galaxy Clusters and its Velocity Features
- A Graphical Interpretation of Circumgalactic Precipitation
- Heating Cold Clumps by Jet-inflated Bubbles in Cooling Flow Clusters
- Characterizing the Uncertainty in Cluster Magnetic Fields derived from Rotation Measures
- Connecting turbulent velocities and magnetic fields in galaxy cluster simulations with active galactic nuclei jets
- Chaotic cold accretion in giant elliptical galaxies heated by AGN cosmic rays
- Cosmic rays and thermal instability in self-regulating cooling flows of massive galaxy clusters
- The Sunyaev-Zel'dovich effect of simulated jet-inflated bubbles in clusters
- Jets, Bubbles, and Heat Pumps in Galaxy Clusters
- Environmental Dependence of Self-Regulating Black-hole Feedback in Massive Galaxies
- NGC 1275: an outlier of the black hole-host scaling relations
- The young radio lobe of 3C 84: inferred gas properties in the central 10 parsec
- Powering of H filaments by cosmic rays
- Thermally Unstable Cooling Stimulated by Uplift: The Spoiler Clusters
- The most massive galaxies with large depleted cores: structural parameter relations and black hole masses
Cited by in corpus (19)
- Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters
- Active galactic nucleus jet feedback in hydrostatic halos
- The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
- EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
- On the origin of star formation quenching in massive galaxies at in the cosmological simulations IllustrisTNG
- Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
- The properties of magnetised cold filaments in a cool-core galaxy cluster
- Accretion onto supermassive and intermediate mass black holes in cosmological simulations
- Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
- Hungry or Not: How Stellar-Mass Black Holes Grow (or Don't) in Dark Matter Mini-Haloes at High-Resolution
- On the impact of AGN feedback modes onto the turbulent properties of the multiphase ICM
- What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
- The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
- Numerical modelling of the lobes of radio galaxies -- Paper V: Universal Pressure Profile cluster atmospheres
- Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster
- Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
- How supermassive black holes shape central entropies in galaxy clusters
- Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at
- On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes