A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion

@article{Gebhardt2000ARB,
  title={A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion},
  author={Karl Gebhardt and Ralf Bender and Gary Allen Bower and Alan Dressler and S. M. Faber and Alexei V. Filippenko and Richard Green and Carl J. Grillmair and Luis C. Ho and John Kormendy and Tod R. Lauer and John Magorrian and Jason Pinkney and Douglas O. Richstone and Scott Tremaine},
  journal={The Astrophysical Journal},
  year={2000},
  volume={539}
}
We describe a correlation between the mass Mbh of a galaxy's central black hole and the luminosity-weighted line-of-sight velocity dispersion σe within the half-light radius. The result is based on a sample of 26 galaxies, including 13 galaxies with new determinations of black hole masses from Hubble Space Telescope measurements of stellar kinematics. The best-fit correlation is Mbh = 1.2(±0.2) × 108 M☉(σe/200 km s-1)3.75 (±0.3) over almost 3 orders of magnitude in Mbh; the scatter in Mbh at… 

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References

SHOWING 1-10 OF 50 REFERENCES
Evidence for a Massive Black Hole in the S0 Galaxy NGC 4342
We present axisymmetric dynamical models of the edge-on S0 galaxy NGC 4342. This small low-luminosity galaxy harbors, in addition to its outer disk, a bright nuclear stellar disk. A combination of
The Demography of massive dark objects in galaxy centers
We construct dynamical models for a sample of 36 nearby galaxies with Hubble Space Telescope (HST) photometry and ground-based kinematics. The models assume that each galaxy is axisymmetric, with a
Evidence for a black hole from high rotation velocities in a sub-parsec region of NGC4258
MANY galaxies are thought to contain massive black holes— exceeding ten million solar masses—at their centres1,2, but firm observational evidence has proved to be surprisingly elusive. The best
A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
The masses of supermassive black holes correlate almost perfectly with the velocity dispersions of their host bulges, Mbh ∝ σα, where α = 4.8 ± 0.5. The relation is much tighter than the relation
Kinematics of the nuclear ionized gas in the radio galaxy m84 (ngc 4374)
We present optical long-slit spectroscopy of the nucleus of the nearby radio galaxy M84 (NGC 4374 = 3C 272.1) obtained with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope.
The Mass Distribution in the Elliptical Galaxy NGC 3377: Evidence for a 2 ? 108 M? Black Hole
This paper is a study of the mass distribution in the central 35'' 1.7 kpc of the E5 galaxy NGC 3377. Stellar rotation velocity and velocity dispersion profiles (seeing σ* = 020-056) and V-band
Nuclear Disks of Gas and Dust in Early-Type Galaxies and the Hunt for Massive Black Holes: Hubble Space Telescope Observations of NGC 6251
We discuss Hubble Space Telescope (HST) optical images and spectra of NGC 6251, a giant E2 galaxy and powerful radio source at a distance of 106 Mpc (for H0=70 km s-1 Mpc-1). The galaxy is known to
Spectroscopic Evidence for a Supermassive Black Hole in NGC 4486B
The stellar kinematics of the low-luminosity elliptical galaxy NGC 4486B have been measured in seeing σ* = 022 with the Canada-France-Hawaii Telescope and Subarcsecond Imaging Spectrograph. Lauer and
Axisymmetric, Three-Integral Models of Galaxies: A Massive Black Hole in NGC 3379
We fit axisymmetric three-integral dynamical models to NGC 3379 using the line-of-sight velocity distribution obtained from Hubble Space Telescope FOS spectra of the galaxy center and ground-based
Evidence for a Supermassive Black Hole in the Nucleus of M31
Stellar rotation velocities and velocity dispersions along three slit positions in M31 have been measured, and three-dimensional velocity and velocity dispersion fields are obtained in order to
...
1
2
3
4
5
...