Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms
arXiv:1412.7660 · doi:10.1051/0004-6361/201425094
Abstract
Using an advanced semi analytic model (SAM) for galaxy formation, we have investigated the statistical effects of assuming two different mechanisms for triggering AGN activity on the properties of AGN host galaxies. We have considered a first accretion mode where AGN activity is triggered by disk instabilities (DI) in isolated galaxies, and a second feeding mode where such an activity is triggered by galaxy mergers and fly-by events (interactions, IT). We obtained the following results:i) for hosts with , both DI and IT modes are able to account for the observed AGN hosts stellar mass function; for more massive hosts, the DI scenario predicts a lower space density than the IT model, lying below the observational estimates for z>0.8.ii) The analysis of the color-magnitude diagram (CMD) of AGN hosts for redshift z < 1.5 can provide a good observational test to effectively discriminate between the DI and IT mode, since DIs are expected to yield AGN host galaxy colors skewed towards bluer colors, while in the IT scenario the majority of hosts are expected to reside in the red sequence.iii) While both IT and DI scenarios can account for AGN triggered in main sequence or starburst galaxies, DIs fail in triggering AGN activity in passive galaxies.iv) The two modes are characterized by a different duration of the AGN phase, with DIs lasting even on time scales Gyr, much longer with respect to the IT scenario.v) The scatter of the relation could represent another crucial diagnostics to discriminate between the two triggering modes, since the DI scenario predicts an appreciably lower scatter of the relation than the IT scenario. vi) Disk instabilities are not able to account for the observed fraction of AGN in groups for z < 1 and clusters for z < 0.7, while the IT scenario provides a good match to observational data.
arXiv commentPaper accepted for publication in section 4. Extragalactic astronomy of Astronomy and Astrophysics
References in corpus (119)
- Stellar population synthesis at the resolution of 2003
- The Global Schmidt Law in Star Forming Galaxies
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- 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
- The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
- A Relationship Between Nuclear Black Hole Mass and Galaxy Velocity Dispersion
- Energy input from quasars regulates the growth and activity of black holes and their host galaxies
- The physical properties of star forming galaxies in the low redshift universe
- The broken hierarchy of galaxy formation
- The Formation of Galactic Disks
- The Cosmic Evolution Survey (COSMOS) -- Overview
- Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
- The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
- Gasdynamics and Starbursts in Major Mergers
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- UV Star Formation Rates in the Local Universe
- On the Black Hole Mass - Bulge Mass Relation
- New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
- The reversal of the star formation-density relation in the distant universe
- Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
- Quantifying the bimodal color-magnitude distribution of galaxies
- Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background
- Revisiting the Scaling Relations of Black Hole Masses and Host Galaxy Properties
- The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
- An Observational Determination of the Bolometric Quasar Luminosity Function
- Cosmological Evolution of the Hard X-ray AGN Luminosity Function and the Origin of the Hard X-ray Background
- Observational constraints on growth of massive black holes
- The Infrared Spectral Energy Distribution of Normal Star-Forming Galaxies: Calibration at Far-Infrared and Submillimeter Wavelengths
- The lesser role of starbursts for star formation at z=2
- Toward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations
- Hubble Space Telescope Images of a Sample of Twenty Nearby Luminous Quasars
- Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs
- How Do Massive Black Holes Get Their Gas?
- The effect of galaxy mass ratio on merger--driven starbursts
- A Close Look at Star Formation around Active Galactic Nuclei
- The HELLAS2XMM survey. VII. The hard X-ray luminosity function of AGN up to z=4: more absorbed AGN at low luminosities and high redshifts
- CANDELS: Constraining the AGN-Merger Connection with Host Morphologies at z~2
- The Evolutionary History of Lyman Break Galaxies Between Redshift 4 and 6: Observing Successive Generations of Massive Galaxies in Formation
- Major Galaxy Mergers Only Trigger the Most Luminous AGN
- The Many Manifestations of Downsizing: Hierarchical Galaxy Formation Models confront Observations
- Two bright submillimeter galaxies in a z=4.05 proto-cluster in GOODS-North, and accurate radio-infrared photometric redshifts
- Kinematic Structure of Merger Remnants
- Black hole variability and the star formation-AGN connection: Do all star-forming galaxies host an AGN?
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- Eddington-limited accretion and the black hole mass function at redshift 6
- The PRIsm MUlti-Object Survey (PRIMUS) I: Survey Overview and Characteristics
- The Fundamental Scaling Relations of Elliptical Galaxies
- The galaxy stellar mass-star formation rate relation: Evidence for an evolving stellar initial mass function?
- Star formation and mass assembly in high redshift galaxies
- PRIMUS: The dependence of AGN accretion on host stellar mass and color
- Formation of z ~ 6 quasars from hierarchical galaxy mergers
- The Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z=2.5: Results from PEP-Herschel
- The contribution of starbursts and normal galaxies to infrared luminosity functions at z < 2
- The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue
- The XMM-Newton Wide-Field Survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous AGN
- An Analytic Model of Angular Momentum Transport by Gravitational Torques: From Galaxies to Massive Black Holes
- AEGIS: The color-magnitude relation for X-ray selected AGN
- Black Hole growth and AGN obscuration by instability-driven inflows in high-redshift disk galaxies fed by cold streams
- GOODS-Herschel: The far-infrared view of star formation in AGN host galaxies since z~3
- Accreting SMBHs in the COSMOS field and the connection to their host galaxies
- The HELLAS2XMM survey: IV. Optical identifications and the evolution of the accretion luminosity in the Universe
- Evolution of Galaxy Stellar Mass Functions, Mass Densities, and Mass to Light Ratios from z 7 to z 4
- The hidden "AGN main sequence": Evidence for a universal black hole accretion to star formation rate ratio since z~2 producing a M_BH-M* relation
- Ongoing and co-evolving star formation in zCOSMOS galaxies hosting Active Galactic Nuclei
- The Evolution of the M-sigma Relation
- AGN Host Galaxies at z~0.4-1.3 : Bulge-dominated and Lacking Merger-AGN Connection
- Mass function of dormant black holes and the evolution of the Active Galactic Nuclei
- The Effects of Gas on Morphological Transformation in Mergers: Implications for Bulge and Disk Demographics
- Accretion-Driven Evolution of Black Holes: Eddington Ratios, Duty Cycles, and Active Galaxy Fractions
- The Blast Wave Model for AGN Feedback: Effects on AGN Obscuration
- A correlation between star formation rate and average black hole accretion in star forming galaxies
- Color-Magnitude Relations of Active and Non-Active Galaxies in the Chandra Deep Fields: High-Redshift Constraints and Stellar-Mass Selection Effects
- The evolution of AGN across cosmic time: what is downsizing?
- The Subaru/XMM-Newton Deep Survey (SXDS): III. X-Ray Data
- The impact of galaxy interactions on AGN activity in zCOSMOS
- The PRIsm MUlti-object Survey (PRIMUS). II. Data Reduction and Redshift Fitting
- Cosmic Evolution of Mass Accretion Rate and Metalicity in Active Galactic Nuclei
- Star formation in AGN hosts in GOODS-N
- Morphologies of z~0.7 AGN Host Galaxies in CANDELS: No trend of merger incidence with AGN luminosity
- The LABOCA survey of the Extended Chandra Deep Field South: Two modes of star formation in AGN hosts?
- Faint high-redshift AGN in the Chandra Deep Field South: the evolution of the AGN luminosity function and black hole demography
- AEGIS: The Clustering of X-ray AGN Relative to Galaxies at z~1
- The Abundance of Distant and Extremely Red Galaxies: The Role of AGN Feedback in Hierarchical Models
- Merger Rate of Equal-Mass Spherical Galaxies
- The VVDS type-1 AGN sample: The faint end of the luminosity function
- The evolution of the specific star formation rate of massive galaxies to z ~ 1.8 in the E-CDFS
- The evolving slope of the stellar mass function at 0.6 <= z < 4.5 from deep WFC3 data
- A Multiwavelength Consensus on the Main Sequence of Star-Forming Galaxies at z~2
- The Mean Star-Forming Properties of QSO Host Galaxies
- The Fall of the Quasar Population
- Origin of the anti-hierarchical growth of black holes
- AEGIS: Host Galaxy Morphologies of X-ray and Infrared-selected AGN at 0.2 < z < 1.2
- The Evolution of Active Galactic Nuclei in Clusters of Galaxies to Redshift 1.3
- Chandra Observations of the Highest Redshift Quasars from the Sloan Digital Sky Survey
- Black-Hole Mass and Growth Rate at z~4.8: A Short Episode of Fast Growth Followed by Short Duty Cycle Activity
- Host galaxy morphologies of X-ray selected AGN: assessing the significance of different black hole fueling mechanisms to the accretion density of the Universe at z~1
- On the puzzling plateau in the specific star formation rate at z=2-7
- Intracluster and Intragroup Entropy from Quasar Activity
- The Evolution of the M_BH-sigma relation Inferred from the Age Distribution of Local Early-Type Galaxies and AGN Evolution
- Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions
- Radiation pressure force and black hole mass determination in low redshift type-I and type-II active galactic nuclei
- AGN Feedback on the Intracluster Medium
- Dust-Corrected Colors Reveal Bimodality in AGN Host Galaxy Colors at z~1
- Early Hierarchical Formation of Massive Galaxies Triggered By Interactions
- First Measurement of a Rapid Increase in the AGN Fraction in High-Redshift Clusters of Galaxies
- The [OIII] emission line luminosity function of optically selected type-2 AGN from zCOSMOS
- The host galaxies of three radio-loud quasars: 3C 48, 3C 345, and B2 1425+267
- The XMM-Newton survey of the ELAIS-S1 field. I: Number counts, angular correlation function and X-ray spectral properties
- Tidal Disruption of Satellite Galaxies in a Semi-Analytic Model of Galaxy Formation
- Active Galactic Nuclei in Groups and Clusters of Galaxies: Detection and Host Morphology
- X-ray selected AGN Hosts are Similar to Inactive Galaxies out to z=3: Results from CANDELS/CDF-S
- A Serendipitous XMM Survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z=0.8 to z=0.1
- A Comprehensive Study of Large Scale Structures in the GOODS-SOUTH Field up to z \sim 2.5
- Mergers and interactions in SDSS type 2 quasars at z~0.3-0.4. SDSS J143027.66-005614.8: a case study
- The interaction-driven starburst contribution to the cosmic star formation rate density
- The evolution of the AGN content in groups up to z~1
- Probing AGN triggering mechanisms through the starburstiness of the host galaxies
Cited by in corpus (13)
- Observational Constraints on the Feeding of Supermassive Black Holes
- Constraints on gamma-ray and neutrino emission from NGC 1068 with the MAGIC telescopes
- The Chandra COSMOS Legacy survey: the z>3 sample
- Extragalactic gamma-ray background from AGN winds and star-forming galaxies in cosmological galaxy formation models
- Determining the radio AGN contribution to the radio-FIR correlation using the black hole fundamental plane relation
- Constraining AGN triggering mechanisms through the clustering analysis of active black holes
- The Relative Growth of Black Holes and of the Stellar Components of Galaxies
- Circumnuclear Structures in Megamaser Host Galaxies
- Intrinsic and observed dual AGN fractions from major mergers
- Astrophysics with the Laser Interferometer Space Antenna
- The detections of inflowing gas from narrow absorption lines at the parsec scale
- A study of interacting galaxies from the Arp-Madore Catalogue: Triggering of star formation and nuclear activity
- Compton-thick AGN Characterisation in a Multi-wavelength Context: Insights from the 70-Month \textit{SWIFT}/BAT Catalogue