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Rotation of the Bulge Components of Disk Galaxies
John Kormendy,G. Illingworth +1 more
- pp 195
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The article was published on 1979-01-01 and is currently open access. It has received 170 citations till now. The article focuses on the topics: Bulge & Rotation.read more
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Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Supplemental Material
John Kormendy,Luis C. Ho +1 more
TL;DR: Kormendy and Ho as mentioned in this paper proposed a method to estimate the BH masses for galaxies with active nuclei (AGNs) based on the observational criteria that are used to classify classical and pseudo bulges.
Journal ArticleDOI
Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
TL;DR: In the far future, evolution will mostly be secular, the slow rearrangement of energy and mass that results from interactions involving collective phenomena such as bars, oval disks, spiral structure, and triaxial dark halos as mentioned in this paper.
Journal ArticleDOI
The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
Kayhan Gültekin,Douglas O. Richstone,Karl Gebhardt,Tod R. Lauer,Scott Tremaine,Monique Aller,Ralf Bender,Alan Dressler,S. M. Faber,Alexei V. Filippenko,Richard F. Green,Luis C. Ho,John Kormendy,John Magorrian,Jason Pinkney,Christos Siopis +15 more
TL;DR: This article derived improved versions of the relations between supermassive black hole mass and host-galaxy bulge velocity dispersion (sigma) and luminosity (L) (the M-sigma and M-L relations), based on 49 M_BH measurements and 19 upper limits.
Journal ArticleDOI
Structure and formation of elliptical and spheroidal galaxies
TL;DR: In this paper, surface photometry of all known elliptical galaxies in the Virgo cluster is combined with published data to derive composite profiles of brightness, ellipticity, position angle, isophote shape, and color over large radius ranges.
Journal ArticleDOI
Beyond the bulge: a fundamental relation between supermassive black holes and dark matter halos
TL;DR: In this paper, the authors investigated whether the masses MBH of supermassive black holes (SBHs) correlate with the total gravitational mass of their host galaxy, or the mass MDM of the dark matter halo in which they presumably formed.
References
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Journal ArticleDOI
Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
John Kormendy,Luis C. Ho +1 more
TL;DR: In this paper, supermassive black holes (BHs) have been found in 85 galaxies by dynamical modeling of spatially resolved kinematics, and it has been shown that BHs and bulges coevolve by regulating each other's growth.
Journal ArticleDOI
Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
TL;DR: In the far future, evolution will mostly be secular, the slow rearrangement of energy and mass that results from interactions involving collective phenomena such as bars, oval disks, spiral structure, and triaxial dark halos as mentioned in this paper.
Journal ArticleDOI
The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
Kayhan Gültekin,Douglas O. Richstone,Karl Gebhardt,Tod R. Lauer,Scott Tremaine,Monique Aller,Ralf Bender,Alan Dressler,S. M. Faber,Alexei V. Filippenko,Richard F. Green,Luis C. Ho,John Kormendy,John Magorrian,Jason Pinkney,Christos Siopis +15 more
TL;DR: This article derived improved versions of the relations between supermassive black hole mass and host-galaxy bulge velocity dispersion (sigma) and luminosity (L) (the M-sigma and M-L relations), based on 49 M_BH measurements and 19 upper limits.
Journal ArticleDOI
Structure and formation of elliptical and spheroidal galaxies
TL;DR: In this paper, surface photometry of all known elliptical galaxies in the Virgo cluster is combined with published data to derive composite profiles of brightness, ellipticity, position angle, isophote shape, and color over large radius ranges.
Journal ArticleDOI
Beyond the bulge: a fundamental relation between supermassive black holes and dark matter halos
TL;DR: In this paper, the authors investigated whether the masses MBH of supermassive black holes (SBHs) correlate with the total gravitational mass of their host galaxy, or the mass MDM of the dark matter halo in which they presumably formed.