A study of the scaling relation $M_{\bullet }\propto R_e{\sigma }^3$ for supermassive black holes and an update of the corresponding theoretical model

Abstract

In this paper we want to compare the theoretical predictions of a law proposed by Feoli and Mancini, with the most recent experimental data about galaxies and Supermassive black holes. The physical principle behind this law is the transformation of the angular momentum of the interstellar material, which falls into the black hole, into the angular momentum of the radiation emitted in this process. Despite the simplicity of the model, this law shows an excellent agreement with the experimental data for early-type galaxies while a new approach is proposed for spirals.

arXiv commentAccepted for publication in Astrophysics and Space Science

References in corpus (61)

• A Fundamental Relation Between Supermassive Black Holes and Their 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 slope of the black-hole mass versus velocity dispersion correlation
• The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
• The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
• Some Aspects of Measurement Error in Linear Regression of Astronomical Data
• On the Maximum Luminosity of Galaxies and Their Central Black Holes: Feedback From Momentum-Driven Winds
• A Physical Model for the Co-evolution of QSOs and of their Spheroidal Hosts
• A unified model for AGN feedback in cosmological simulations of structure formation
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
• Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research
• A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes
• Beyond the Bulge: a Fundamental Relation Between Supermassive Black Holes and Dark Matter Halos
• The M(BH)-Sigma Relation for Supermassive Black Holes
• Self-Regulated Growth of Supermassive Black Holes in Galaxies as the Origin of the Optical and X-ray Luminosity Functions of Quasars
• An expanded M_bh-sigma diagram, and a new calibration of active galactic nuclei masses
• The SINFONI Black Hole Survey: The Black Hole Fundamental Plane revisited and the paths of (co-) evolution of supermassive black holes and bulges
• Grand unification of AGN activity in the LambdaCDM cosmology
• Unification of the Fundamental Plane and Super-Massive Black Holes Masses
• The black hole mass -- stellar velocity dispersion correlation: bulges versus pseudobulges
• Black Holes in Astrophysics
• Radiative feedback from quasars and the growth of massive black holes in stellar spheroids
• The Fundamental Plane of Accretion Onto Black Holes with Dynamical Masses
• An Observed Fundamental Plane Relation for Supermassive Black Holes
• A Theoretical Interpretation of the Black Hole Fundamental Plane
• Fundamental Planes, and the "barless" M-sigma relation, for supermassive black holes
• Black Holes and Hosts of Active and Quiescent Galaxies: I. The Black Hole-Bulge Relation revisited
• Observational evidence for a connection between supermassive black holes and dark matter haloes
• A 17-billion-solar-mass black hole in a group galaxy with a diffuse core
• Feedback from central black holes in elliptical galaxies. I: models with either radiative or mechanical feedback but not both
• On The Linearity of The Black Hole - Bulge Mass Relation in Active and in Nearby Galaxies
• Supermassive black holes do not correlate with dark matter halos of galaxies
• On the Correlations of Massive Black Holes with their Host Galaxies
• Host Galaxy Bulge Predictors of Supermassive Black Hole Mass
• The First Massive Black Hole Seeds and Their Hosts
• Star Formation-Regulated Growth of Black Holes in Protogalactic Spheroids
• A correlation between central supermassive black holes and the globular cluster systems of early-type galaxies
• Reasoning From Fossils: Learning From the Local Black Hole Population About the Evolution of Quasars
• Self-regulated black hole accretion, the M-sigma relation, and the growth of bulges in galaxies
• How important is the dark matter halo for black hole growth?
• Upper Limits on the Masses of 105 Supermassive Black Holes from Hubble Space Telescope/Space Telescope Imaging Spectrograph Archival Data
• Evidence for recent star formation in BCGs: a correspondence between blue cores and UV excess
• Relic Black Holes In Galactic Nuclei
• Supermassive black holes, star formation and downsizing of elliptical galaxies
• Correlation of Black Hole and Bulge Masses: Driven by Energy but Correlated with Momentum
• Feedback from central black holes in elliptical galaxies. II: Can purely mechanical energy feedback models work?
• Quasar Clustering in Cosmological Hydrodynamic Simulations: Evidence for mergers
• A HR-like diagram for galaxies: the M_BH versus M_G sigma^2 relation
• Is there a relationship between the mass of a SMBH and the kinetic energy of its host elliptical galaxy?
• Relation Between Globular Clusters and Supermassive Black Holes in Ellipticals as a Manifestation of the Black Hole Fundamental Plane
• The scaling relation between the mass of supermassive black holes and the kinetic energy of random motions of the host galaxies
• Environmental effects on the growth of super massive black holes and AGN feedback
• Improved tests on the relationship between the kinetic energy of galaxies and the mass of their central black holes
• Correlation of Black Hole-Bulge Masses by AGN Jets
• The SMBH mass versus M_G sigma^2 relation: A comparison between real data and numerical models
• The correlation of black hole mass with metallicity index of host spheroid
• A fundamental equation for Supermassive Black Holes

Cited by in corpus (3)

• A note on the interpretation of the statistical analysis of the $M_{\bullet }-M_G{\sigma }^2$ scaling relation
• An updated comparison of the $M_{\bullet }$ vs $M_G{\sigma }^2$ relation with $M_{\bullet }$ vs $\sigma$ and the problem of the masses of galaxies
• Jet-driven active galactic nucleus feedback in galaxy formation before black hole formation