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 between Mbh and bulge luminosity, with a scatter no larger than expected on the basis of measurement error alone. Black hole masses recently estimated by Magorrian et al. lie systematically above the Mbh-σ relation defined by more accurate mass estimates, some by as much as 2 orders of magnitude. The tightness of the Mbh-σ relation implies a strong link between black hole formation and the properties of the stellar bulge.

[1]  E.P.J. van den Heuvel,et al.  Black holes in binaries and galactic nuclei , 2001 .

[2]  G. Mamon,et al.  Dynamics of Galaxies: From the Early Universe to the Present , 2000 .

[3]  M. Merrifield,et al.  The black hole mass-galaxy age relation , 2000, astro-ph/0002350.

[4]  G. Kauffmann,et al.  A unified model for the evolution of galaxies and quasars , 1999, astro-ph/9906493.

[5]  S. Chakrabarti.  Observational Evidence for Black Holes in the Universe , 2008 .

[6]  S. Tremaine,et al.  Axisymmetric, Three-Integral Models of Galaxies: A Massive Black Hole in NGC 3379 , 1999, astro-ph/9912026.

[7]  J. M. Moran,et al.  A geometric distance to the galaxy NGC4258 from orbital motions in a nuclear gas disk , 1999, Nature.

[8]  Garth D. Illingworth,et al.  The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XXVI. The Calibration of Population II Secondary Distance Indicators and the Value of the Hubble Constant , 1999, astro-ph/9908192.

[9]  H. Ford,et al.  Nuclear Disks of Gas and Dust in Early-Type Galaxies and the Hunt for Massive Black Holes: Hubble Space Telescope Observations of NGC 6251 , 1998, astro-ph/9811319.

[10]  R. Bacon,et al.  Dynamical models of ngc 3115 , 1998, astro-ph/9810306.

[11]  L. Ho.  Supermassive Black Holes in Galactic Nuclei , 1998, astro-ph/9803307.

[12]  M. Valluri,et al.  Galaxy Dynamics , 1999 .

[13]  L. Ho.  in Observational Evidence for Black Holes in the Universe , 1999 .

[14]  J. Barnes,et al.  Galaxy Interactions at Low and High Redshift , 1999 .

[15]  D. Schlegel,et al.  Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .

[16]  F. V. D. Bosch,et al.  NUCLEAR STELLAR DISCS IN EARLY-TYPE GALAXIES - II. PHOTOMETRIC PROPERTIES , 1998, astro-ph/9806078.

[17]  S. Tremaine,et al.  The Demography of Massive Dark Objects in Galaxy Centers , 1997, astro-ph/9708072.

[18]  M. Rees,et al.  High-redshift galaxies, their active nuclei and central black holes , 1997, astro-ph/9712259.

[19]  D. Schlegel,et al.  Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.

[20]  W. Sparks,et al.  The Supermassive Black Hole of M87 and the Kinematics of Its Associated Gaseous Disk , 1997, astro-ph/9706252.

[21]  P. T. de Zeeuw,et al.  Improved Evidence for a Black Hole in M32 from HST/FOS Spectra. II. Axisymmetric Dynamical Models , 1997, astro-ph/9705081.

[22]  Timothy M. Heckman,et al.  The Nuclear Ionized Gas in the Radio Galaxy M84 (NGC 4374) , 1997, astro-ph/9710264.

[23]  J. Newman,et al.  Measurement of an Active Galactic Nucleus Central Mass on Centiparsec Scales: Results of Long-Term Optical Monitoring of Arp 102B , 1997, astro-ph/9703023.

[24]  H. Ford,et al.  Evidence for a Massive Black Hole in the Active Galaxy NGC 4261 from Hubble Space Telescope Images and Spectra , 1996 .

[25]  Matthew A. Bershady,et al.  Linear Regression for Astronomical Data with Measurement Errors and Intrinsic Scatter , 1996, astro-ph/9605002.

[26]  I. Jørgensen,et al.  Spectroscopy for E and S0 galaxies in nine clusters , 1995 .

[27]  John Kormendy,et al.  Inward Bound—The Search for Supermassive Black Holes in Galactic Nuclei , 1995 .

[28]  Naomasa Nakai,et al.  Evidence for a black hole from high rotation velocities in a sub-parsec region of NGC4258 , 1995, Nature.

[29]  S. Kent,et al.  Galactic structure from the Spacelab Infrared Telescope. III: A dynamical model for the Milky Way bulge , 1992 .

[30]  R. Terlevich,et al.  On the behaviour of the IR CA II triplet in normal and active galaxies , 1990 .

[31]  J. Mathis,et al.  The relationship between infrared, optical, and ultraviolet extinction , 1989 .

[32]  David Burstein,et al.  Spectroscopy and photometry of elliptical galaxies. II - The spectroscopic parameters , 1987 .

[33]  S. Djorgovski,et al.  Fundamental Properties of Elliptical Galaxies , 1987 .

[34]  S. Faber.  Nearly Normal Galaxies , 1987 .

[35]  S. Faber,et al.  Global Scaling Relations for Elliptical Galaxies and Implications for Formation , 1987 .

[36]  G. Vaucouleurs,et al.  Systematics of Bulge-to-Disk Ratios , 1986 .

[37]  T. Heckman,et al.  The kinematics of stars and gas in radio galaxies , 1985 .

[38]  W. Jefferys.  On the method of least squares , 1980 .

[39]  G. Vaucouleurs,et al.  An outsider's view of the Galaxy: photometric parameters, scale lengths, and absolute magnitudes of the spheroidal and disk components of our Galaxy. , 1978 .