Relation Between Globular Clusters and Supermassive Black Holes in Ellipticals as a Manifestation of the Black Hole Fundamental Plane

Abstract

We analyze the relation between the mass of the central supermassive black hole (Mbh) and the number of globular clusters (Ngc) in elliptical galaxies and bulges as a ramification of the black hole fundamental plane, the theoretically predicted and observed multi-variable correlation between Mbh and bulge binding energy. Although the tightness of the Mbh-Ngc correlation suggests an unlikely causal link between supermassive black holes and globular clusters, such a correspondence can exhibit small scatter even if the physical relationship is indirect. We show that the relatively small scatter of the Mbh-Ngc relation owes to the mutual residual correlation of Mbh and Ngc with stellar mass when the velocity dispersion is held fixed. Thus, present observations lend evidence for feedback-regulated models in which the bulge binding energy is most important; they do not necessarily imply any `special' connection between globular clusters and Mbh. This raises the question of why Ngc traces the formation of ellipticals and bulges sufficiently well to be correlated with binding energy.

7 pages, 2 figures, accepted for publication in ApJL

References in corpus (37)

• 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
• Modeling feedback from stars and black holes in galaxy mergers
• The Relation between Black Hole Mass, Bulge Mass, and Near-Infrared Luminosity
• The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
• An Observational Determination of the Bolometric Quasar Luminosity Function
• Structure and Formation of Elliptical and Spheroidal Galaxies
• Linear Regression for Astronomical Data with Measurement Errors and Intrinsic Scatter
• A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
• Kinematic Structure of Merger Remnants
• A Correlation between Galaxy Light Concentration and Supermassive Black Hole Mass
• The ACS Virgo Cluster Survey XV. The Formation Efficiencies of Globular Clusters in Early-Type Galaxies: The Effects of Mass and Environment
• New Insights from HST Studies of Globular Cluster Systems I: Colors, Distances and Specific Frequencies of 28 Elliptical Galaxies
• The ACS Virgo Cluster Survey. I. Introduction to the Survey
• Fueling Low-Level AGN Activity Through the Stochastic Accretion of Cold Gas
• The Efficiency of Globular Cluster Formation
• Dissipation and Extra Light in Galactic Nuclei: II. 'Cusp' Ellipticals
• Equal- and unequal-mass mergers of disk and elliptical galaxies with black holes
• The Centers of Early-Type Galaxies with HST. VI. Bimodal Central Surface Brightness Profiles
• The Evolution of the M-sigma Relation
• An Observed Fundamental Plane Relation for Supermassive Black Holes
• A Theoretical Interpretation of the Black Hole Fundamental Plane
• Dissipation and Extra Light in Galactic Nuclei: I. Gas-Rich Merger Remnants
• Binding Energy and the Fundamental Plane of Globular Clusters
• Dissipation and Extra Light in Galactic Nuclei: III. 'Core' Ellipticals and 'Missing' Light
• Host Galaxy Bulge Predictors of Supermassive Black Hole Mass
• 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
• The connection between globular cluster systems and their host galaxy and environment: a case study of the isolated elliptical NGC 821
• Globular Clusters in Dense Clusters of Galaxies
• The Small Scatter in BH-Host Correlations & The Case for Self-Regulated BH Growth
• The Globular Cluster/Central Black Hole Connection in Galaxies
• A HR-like diagram for galaxies: the M_BH versus M_G sigma^2 relation

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• Global Properties of `Ordinary' Early-type Galaxies: photometry and spectroscopy of stars and globular clusters in NGC 4494
• Do We Expect Most AGN to Live in Disks?
• GASP XXIV. The history of abruptly quenched galaxies in clusters
• Globular clusters and supermassive black holes in galaxies: further analysis and a larger sample
• The Overlooked Potential of Generalized Linear Models in Astronomy-III: Bayesian Negative Binomial Regression and Globular Cluster Populations
• Exploring the Correlations between Globular Cluster Populations and Supermassive Black Holes in Giant Galaxies
• The SLUGGS survey: Probing the supermassive black hole connection with bulges and haloes using red and blue globular cluster systems
• The scaling relation between the mass of supermassive black holes and the kinetic energy of random motions of the host galaxies
• The relation between globular cluster systems and supermassive black holes in spiral galaxies. The case study of NGC 4258
• M - sigma relation between SMBHs and the velocity dispersion of globular cluster systems
• Dark halo microphysics and massive black hole scaling relations in galaxies
• 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
• A note on the interpretation of the statistical analysis of the $M_{\bullet }-M_G{\sigma }^2$ scaling relation