The relation between accretion rate and jet power in early-type galaxies with thermally unstable hot atmospheres

Abstract

We use Chandra X-ray data and Very Large Array radio observations for a sample of 20 nearby, massive, X-ray bright, early-type galaxies to investigate the relation between the Bondi accretion rates and the mechanical jet powers. We find a strong correlation ($\rho =0.96_{-0.09}^{+0.03}$; BF${}_{10}>100$) between the Bondi accretion power, $P_{\text{Bondi}}$, and the mechanical jet power, $P_{\text{jet}}$, for a subsample of 14 galaxies, which also host cool H$\alpha$+[NII] line emitting gas and thus likely have thermally unstable atmospheres. The relation between the Bondi accretion power and the mechanical jet power for this subsample is well described by a power-law model $\log \frac{P_{\mathrm{Bondi}}}{10^{43}\mathrm{erg}{\mathrm{s}}^{-1}}=\alpha +\beta \log \frac{P_{\mathrm{jet}}}{10^{43}\mathrm{erg}{\mathrm{s}}^{-1}}$, where $\alpha =1.10\pm 0.25$ and $\beta =1.10\pm 0.24$ with an intrinsic scatter $\sigma =0.08_{-0.06}^{+0.14}$ dex. The results indicate that in all galaxies with thermally unstable atmospheres the cooling atmospheric gas feeds the central black holes at a similar jet-to-Bondi power ratio. For the full sample of 20 galaxies, the correlation is weaker and in a subset of galaxies with no signs of H$\alpha$+[NII] emission, we see a hint for a systematically lower jet-to-Bondi power ratio. We also investigate the dependence of jet power on individual quantities in the Bondi formula such as the supermassive black hole mass ($M_{\bullet }$) and the specific entropy of the gas ($K$) at the Bondi radius. For the subsample of H$\alpha$+[NII] emitting galaxies, we find a very tight correlation of $P_{\text{jet}}$ with $M_{\bullet }$ ($\rho =0.91_{-0.11}^{+0.06}$; BF${}_{10}>100$) and, although poorly constrained, a hint of an anti-correlation for $P_{\text{jet}}$ and $K$ ($\rho =-0.47_{-0.37}^{+0.60}$; BF${}_{10}=1.1$).

arXiv commentaccepted for publication in MNRAS

References in corpus (66)

• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• Observational Evidence of AGN Feedback
• First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
• HI4PI: A full-sky HI survey based on EBHIS and GASS
• Some Aspects of Measurement Error in Linear Regression of Astronomical Data
• The synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era
• HyperLEDA. III. The catalogue of extragalactic distances
• Cosmicflows-2: The Data
• 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
• Updated Atomic Data and Calculations for X-ray Spectroscopy
• The ACS Fornax Cluster Survey. V. Measurement and Recalibration of Surface Brightness Fluctuations and a Precise Value of the Fornax--Virgo Relative Distance
• The relation between accretion rate and jet power in X-ray luminous elliptical galaxies
• The Expanded Very Large Array -- a New Telescope for New Science
• Cooling Flows as a Calorimeter of AGN Mechanical Power
• Thermal Instability in Gravitationally-Stratified Plasmas: Implications for Multi-Phase Structure in Clusters and Galaxy Halos
• Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets
• Accretion onto the Supermassive Black Hole in M87
• The SINFONI Black Hole Survey: The Black Hole Fundamental Plane revisited and the paths of (co-) evolution of supermassive black holes and bulges
• Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations
• Kinematics of the Local Universe XIII. 21-cm line measurements of 452 galaxies with the Nançay radiotelescope, JHK Tully-Fisher relation and preliminary maps of the peculiar velocity field
• A statistical test for Nested Sampling algorithms
• A new radiative cooling curve based on an up to date plasma emission code
• Collaborative Nested Sampling: Big Data vs. complex physical models
• The New Emerging Model for the Structure of Cooling Cores in Clusters of Galaxies
• X-ray Spectral Properties of Low-Mass X-ray Binaries in Nearby Galaxies
• Radiative efficiency, variability and Bondi accretion onto massive black holes: from mechanical to quasar feedback in brightest cluster galaxies
• Chandra X-ray Imaging and Spectroscopy of the M87 Jet and Nucleus
• X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: Tracing the evolution of AGN feedback in clusters of galaxies out to z=1.2
• A 17-billion-solar-mass black hole in a group galaxy with a diffuse core
• Inside the Bondi radius of M87
• Cooling Time, Freefall Time, and Precipitation in the Cores of ACCEPT Galaxy Clusters
• Are Radio AGN Powered by Accretion or Black Hole Spin?
• The Expanded Very Large Array
• The X-ray Halo Scaling Relations of Supermassive Black Holes
• A Synthesis of Data from Fundamental Plane and Surface Brightness Fluctuation Surveys
• Hot Atmospheres, Cold Gas, AGN Feedback and the Evolution of Early Type Galaxies: a Topical Perspective
• The Onset of Thermally Unstable Cooling from the Hot Atmospheres of Giant Galaxies in Clusters - Constraints on Feedback Models
• Cycling of the powerful AGN in MS 0735.6+7421 and the duty cycle of radio AGN in Clusters
• Detection of Radial Surface Brightness Fluctuation and Color Gradients in elliptical galaxies with ACS
• ALMA observations of molecular clouds in three group centered elliptical galaxies: NGC 5846, NGC 4636, and NGC 5044
• Thermodynamic properties, multiphase gas and AGN feedback in a large sample of giant ellipticals
• On the Structure of Hot Gas in Halos: Implications for the Lx-Tx Relation & Missing Baryons
• Resolving the Bondi Accretion Flow toward the Supermassive Black Hole of NGC 3115 with Chandra
• Black Hole Mass Measurements of Radio Galaxies NGC 315 and NGC 4261 Using ALMA CO Observations
• A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics
• The wide-field VLBA calibrator survey -- WFCS
• The Megasecond Chandra XVP Observation of NGC 3115: Witnessing the Flow of Hot Gas within the Bondi Radius
• Connecting Dark Matter Halos with the Galaxy Center and the Supermassive Black Hole
• A systematic search for X-ray cavities in galaxy clusters, groups, and elliptical galaxies
• The Fate of Stellar Mass Loss in Central Cluster Galaxies
• A Relationship Between Halo Mass, Cooling, AGN Heating, and the Coevolution of Massive Black Holes
• Constraints on the Thermal Contents of the X-ray Cavities of Cluster MS 0735.6+7421 with Sunyaev-Zel'dovich Effect Observations
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• VLA Observations of HI in the Circumstellar Envelopes of Asymptotic Giant Branch Stars
• The imprints of AGN feedback within a supermassive black hole's sphere of influence
• Correlations between supermassive black holes, hot atmospheres, and the total masses of early type galaxies
• Synthetic Observations of Simulated AGN Jets: X-ray Cavities
• VLA Radio Study of a Sample of Nearby X-ray and Optically Bright Early-Type Galaxies
• Ultramassive black holes in the most massive galaxies: $M_{\mathrm{BH}}-\sigma$ versus $M_{\mathrm{BH}}-R_{\mathrm{b}}$
• Radio Mode Outbursts in Giant Elliptical Galaxies
• Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296
• Observational Evidence for Enhanced Black Hole Accretion in Giant Elliptical Galaxies
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XII. Ionised gas emission in the inner regions of lenticular galaxies
• A new feedback cycle in the archetypal cooling flow group NGC 5044
• Black hole feedback and the evolution of massive early-type galaxies

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