Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei

Abstract

We review the properties of the established Scaling Relations (SRs) of galaxies and active galactic nuclei (AGN), focusing on their origin and expected evolution back in time, providing a short history of the most important progresses obtained up to now and discussing the possible future studies. We also try to connect the observed SRs with the physical mechanisms behind them, examining to what extent current models reproduce the observational data. The emerging picture clarifies the complexity intrinsic to the galaxy formation and evolution process as well as the basic uncertainties still affecting our knowledge of the AGN phenomenon. At the same time, however, it suggests that the detailed analysis of the SRs can profitably contribute to our understanding of galaxies and AGN.

arXiv comment116, 15 figures

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• Choirs HI Galaxy Groups: The metallicity of dwarf galaxies
• Evidence of bar--driven secular evolution in the gamma--ray narrow--line Seyfert 1 galaxy FBQS J164442.5+261913
• Extreme Gaseous Outflows in Radio-Loud Narrow-Line Seyfert 1 Galaxies
• Simulating the formation and evolution of galaxies: Multi-phase description of the interstellar medium, star formation, and energy feedback
• Slim accretion disks around black holes
• Bulge-Disk Decompositions and Structural Bimodality of Ursa Major Cluster Spiral Galaxies
• The host galaxies of z=7 quasars: predictions from the BlueTides simulation
• On the origin of the Tully-Fisher relation
• Classification and redshift estimation by principal component analysis
• Panchromatic Properties of the Extreme FeII Emitter PHL 1092
• Quasars and their emission lines as cosmological probes
• Fe III emission in quasars: evidence for a dense turbulent medium
• The Host Galaxy of the Quasar HE 0450-2958
• AGN disks and black holes on the weighting scales
• The Black Hole and Central Stellar Population of MCG--6-30-15
• A SuperMassive Black Hole Fundamental Plane for Ellipticals
• Host Galaxies of z=4 Quasars
• Detection of spatial correlations of fundamental plane residuals, and cosmological implications
• Resolving the Interstellar Medium in Ultraluminous Infrared QSO Hosts with ALMA
• X-ray properties of dust-obscured galaxies with broad optical/UV emission lines
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• On Spin Dependence of the Fundamental Plane of Black Hole Activity
• The hybrid solution for the Fundamental Plane
• AGN Broad Line Region variability in the context of Eigenvector 1: case of NGC 5548
• An evolutionary missing link? A modest-mass early-type galaxy hosting an over-sized nuclear black hole
• Spectropolarimetry of low redshift Quasars: origin of the polarization and implications for black hole mass estimates
• Galaxy And Mass Assembly (GAMA): The unimodal nature of the dwarf galaxy population
• The intrinsic dispersion of the Faber-Jackson relation for early-type galaxies as function of the mass and redshift
• Fingerprints of the hierarchical building up of the structure on the gas kinematics of galaxies
• Smoke on the water: CO and H2O in a circumnuclear disc around a quasar at redshift 2.64
• Estimating supermassive black hole masses in AGNs using polarization of broad MgII, H$\alpha$ and H$\beta$ lines
• Strong Evolution in the Luminosity-Velocity Relation at z>1?
• The black hole - host galaxy relation for very low-mass quasars
• On the use of scaling relations for the Tolman test
• Resolving the dynamical mass of a z~1.3 QSO host galaxy using SINFONI and Laser Guide Star assisted Adaptive Optics
• Analysis of the galaxy size versus stellar mass relation
• The environment and redshift dependence of accretion onto dark matter halos and subhalos
• Our Search for an H-R Diagram of Quasars
• The radio-loud narrow-line Seyfert 1 galaxy 1H 0323+342 in a galaxy merger
• On the dynamics of clouds in the broad-line region of AGNs with an ADAF atmosphere
• VLT/SINFONI study of black hole growth in high redshift radio-loud quasars from the CARLA survey
• Supermassive Black Hole Demographics: Evading $M-\sigma$
• How non-linear scaling relations unify dwarf and giant elliptical galaxies
• Is there a connection between Broad Absorption Line Quasars and Narrow Line Seyfert 1 galaxies?
• Evolution of the colour-magnitude relation of early-type galaxies in distant clusters
• The Origin of the Mass-Radius Relation of Early-Type Galaxies
• A Closer Look at Two of the Most Luminous Quasars in the Universe
• Spectro-photometric Evolution of Elliptical Galaxies. II. Models with infall
• Probing early-type galaxy evolution with the Kormendy relation
• CIV Emission as a Probe of Accretion Disk Winds
• Analyzing temporal variations of AGN emission line profiles in the context of (dusty) cloud structure formation in the broad line region
• Selection of highly-accreting quasars: Spectral properties of FeII emitters not belonging to extreme Population A
• Constraints on Galaxy Formation from the Tully-Fisher Relation

Cited by in corpus (1)

• The Main Sequence of quasars: the taming of the extremes