• Corpus ID: 118233492

# Comments on Kormendy, Bender & Cornell (2011, Nature, 469, 374)

@article{Graham2011CommentsOK,
title={Comments on Kormendy, Bender \& Cornell (2011, Nature, 469, 374)},
author={Alister W. Graham},
journal={arXiv: Cosmology and Nongalactic Astrophysics},
year={2011}
}
• A. Graham
• Published 1 March 2011
• Physics
• arXiv: Cosmology and Nongalactic Astrophysics
Comments on Kormendy, Bender & Cornell's (2011, Nature, 469, 374) article "Supermassive black holes do not correlate with galaxy disks or pseudobulges" are provided. A number of scientific concerns regarding the data analysis and conclusions are discussed. A broader historical perspective - difficult for authors to supply within the confines of a Nature article - is also provided.
3 Citations
The scaling relation between the mass of supermassive black holes and the kinetic energy of random motions of the host galaxies
• Physics
• 2012
Context. Thanks to the improved angular resolution of modern telescopes and kinematic models, the existence of supermassive black holes (SMBHs) in the inner part of galaxies, regardless their
THE M BH-L SPHEROID RELATION AT HIGH AND LOW MASSES, THE QUADRATIC GROWTH OF BLACK HOLES, AND INTERMEDIATE-MASS BLACK HOLE CANDIDATES
• Physics
• 2012
From a sample of 72 galaxies with reliable supermassive black hole masses M bh, we derive the M bh-(host spheroid luminosity, L) relation for (1) the subsample of 24 core-Sersic galaxies with
A review of elliptical and disc galaxy structure, and modern scaling laws
A century ago, in 1911 and 1913, Plummer and then Reynolds introduced their models to describe the radial distribution of stars in `nebulae'. This article reviews the progress since then, providing

## References

SHOWING 1-6 OF 6 REFERENCES
Fundamental Planes and the Barless MBH-σ Relation for Supermassive Black Holes
The residuals about the standard Mbh-σ relation correlate with the effective radius, absolute magnitude, and Sersic index of the host bulge, giving rise to an apparent black hole "fundamental plane."
Populating the Galaxy Velocity Dispersion: Supermassive Black Hole Mass Diagram, A Catalogue of (M bh, σ) Values
• A. Graham
• Physics
Publications of the Astronomical Society of Australia
• 2008
Abstract An updated catalogue of 76 galaxies, with direct measurements of supermassive black-hole mass (M bh) plus, when available, the central velocity dispersion (σ0) of their host bulge is
An expanded Mbh–σ diagram, and a new calibration of active galactic nuclei masses
• Physics
• 2010
We present an updated and improved Mbh–σ diagram containing 64 galaxies for which Mbh measurements (not just upper limits) are available. Because of new and increased black hole masses at the
The M_bh-sigma diagram, and the offset nature of barred active galaxies
• Physics
• 2009
From a sample of 50 predominantly inactive galaxies with direct supermassive black hole mass measurements, it has recently been established that barred galaxies tend to reside rightward of the
How Non-Linear Scaling Relations Unify Dwarf and Giant Elliptical Galaxies
Dwarf elliptical galaxies are frequently excluded from bright galaxy samples because they do not follow the same linear relations in diagrams involving effective half light radii, R e , or mean
The black hole mass -- stellar velocity dispersion correlation: bulges versus pseudobulges
We have investigated the correlation between the supermassive black holes (SMBHs) mass ($M_{\rm bh}$) and the stellar velocity dispersion ($\sigma_*$) in two types of host galaxies: the classical