On Spin Dependence of the Fundamental Plane of Black Hole Activity
arXiv:2002.11778 · doi:10.1093/mnras/staa1119
Abstract
The Fundamental Plane (FP) of Black Hole (BH) Activity in galactic nuclei relates X-ray and radio luminosities to BH mass and accretion rate. However, there is a large scatter exhibited by the data, which motivated us for a new variable. We add BH spin as a new variable and estimate the spin dependence of the jet power and disk luminosity in terms of radio and X-ray luminosities. We assume the Blandford-Znajek process as the main source of the outflow, and find that the jet power depends on BH spin stronger than quadratically at moderate and large spin values. We perform a statistical analysis for 10 AGNs which have sub-Eddington accretion rates and whose spin values are measured independently via the reflection or continuum-fitting methods, and find that the spin-dependent relation describes the data significantly better. This analysis, if supported with more data, could imply not only the spin dependence of the FP relation, but also the Blandford-Znajek process in AGN jets.
arXiv commentAccepted for publication in MNRAS
References in corpus (50)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- Advection-Dominated Accretion: A Self-Similar Solution
- Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database
- Advection-Dominated Accretion: Underfed Black Holes and Neutron Stars
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- A fundamental plane of black hole activity
- Relativistic Jets in Active Galactic Nuclei
- A Scheme to Unify Low-Power Accreting Black Holes - Jet-Dominated Accretion Flows and the Radio/X-Ray Correlation
- Thermal Equilibria of Accretion Disks
- A Measurement of the Electromagnetic Luminosity of a Kerr Black Hole
- Black Hole Spin and the Radio Loud/Quiet Dichotomy of Active Galactic Nuclei
- Radio-Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications
- A relationship between AGN jet power and radio power
- The Non-Linear Dependence of Flux on Black Hole Mass and Accretion Rate in Core Dominated Jets
- The distribution and cosmic evolution of massive black hole spins
- Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets
- Suzaku observations of 'bare' active galactic nuclei
- A rapidly spinning supermassive black hole at the centre of NGC 1365
- Measuring the kinetic power of AGN in the radio mode
- Using the Fundamental Plane of Black Hole Activity to Distinguish X-ray Processes from Weakly Accreting Black Holes
- The Spin of the Supermassive Black Hole in NGC 3783
- The Fundamental Plane of Accretion Onto Black Holes with Dynamical Masses
- Refining the fundamental plane of accreting black holes
- Magnetically Driven Accretion Flows in the Kerr Metric II: Structure of the Magnetic Field
- Jet-dominated advective systems: radio and X-ray luminosity dependence on the accretion rate
- Measurement of the spin of the M87 black hole from its observed twisted light
- Measuring Supermassive Black Hole Spins in Active Galactic Nuclei
- Disk-Jet Connection in the Radio Galaxy 3C 120
- General Relativistic Modeling of Magnetized Jets from Accreting Black Holes
- Narrow Iron K Lines in Active Galactic Nuclei: Evolving Populations?
- Black Hole Spin and Accretion Disk Magnetic Field Strength Estimates for more than 750 AGN and Multiple GBH
- An X-Ray View of the Jet-Cycle in the Radio Loud AGN 3C120
- A selection effect boosting the contribution from rapidly spinning black holes to the Cosmic X-ray Background
- The Black Hole Mass of NGC 4151. II. Stellar Dynamical Measurement from Near-Infrared Integral Field Spectroscopy
- Multi-epoch X-ray observations of the Seyfert 1.2 galaxy Mrk 79: bulk motion of the illuminating X-ray source
- The Fundamental Plane of Black Hole Activity in the Optical Band
- Discovery of Millimeter-Wave Excess Emission in Radio-Quiet Active Galactic Nuclei
- The mm-wave compact component of AGN
- A Physical Link Between Jet Formation and Hot Plasma in Active Galactic Nuclei
- A Low-Flux State in IRAS 00521-7054 seen with NuSTAR and XMM-Newton: Relativistic Reflection and an Ultrafast Outflow
- A possible ultra strong and broad Fe Ka emission line in Seyfert 2 galaxy IRAS 00521-7054
- The mass fraction of AGN and the Fundamental Plane of black hole activity from a large X-ray selected sample of LINERs
- Scale-invariant radio jets and varying black hole spin
- Near-infrared observations of star formation and gas flows in the NUGA galaxy NGC 1365
- Revisit Short Term X-ray Spectral Variability of NGC 4151 with Chandra
- Spin Properties of Supermassive Black Holes with Powerful Outflows
- Relationship between X-ray spectral index and X-ray Eddington ratio for Mrk 335 and Ark 564
- A New Radio Loudness Diagnostic for Active Galaxies: a Radio-To-Mid-Infrared Parameter
- Winds and feedback from supermassive black holes accreting at low rates: Hydrodynamical treatment
Cited by in corpus (8)
- On the diversity of the jet production efficiency in Swift/BAT AGNs
- Possible Evidence of a Universal Radio/X-ray Correlation in a near-Complete Sample of Hard X-ray Selected Seyfert Galaxies
- Getting More Out of Black Hole Superradiance: a Statistically Rigorous Approach to Ultralight Boson Constraints from Black Hole Spin Measurements
- Astrophysics with the Laser Interferometer Space Antenna
- Properties of Ultralight Bosons from Spins of Heavy Quasars via Superradiance
- The Jet-Disk Coupling of Seyfert Galaxies from a Complete Hard X-ray Sample
- AGN dichotomy beyond radio loudness: a Gaussian Mixture Model analysis
- Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei