scholarly journals DEPLETED GALAXY CORES AND DYNAMICAL BLACK HOLE MASSES

2013 ◽  
Vol 146 (6) ◽  
pp. 160 ◽  
Author(s):  
S. P. Rusli ◽  
P. Erwin ◽  
R. P. Saglia ◽  
J. Thomas ◽  
M. Fabricius ◽  
...  
2019 ◽  
Vol 15 (S359) ◽  
pp. 37-39
Author(s):  
Benjamin L. Davis ◽  
Nandini Sahu ◽  
Alister W. Graham

AbstractOur multi-component photometric decomposition of the largest galaxy sample to date with dynamically-measured black hole masses nearly doubles the number of such galaxies. We have discovered substantially modified scaling relations between the black hole mass and the host galaxy properties, including the spheroid (bulge) stellar mass, the total galaxy stellar mass, and the central stellar velocity dispersion. These refinements partly arose because we were able to explore the scaling relations for various sub-populations of galaxies built by different physical processes, as traced by the presence of a disk, early-type versus late-type galaxies, or a Sérsic versus core-Sérsic spheroid light profile. The new relations appear fundamentally linked with the evolutionary paths followed by galaxies, and they have ramifications for simulations and formation theories involving both quenching and accretion.


1998 ◽  
Vol 500 (2) ◽  
pp. 642-659 ◽  
Author(s):  
Kiyoshi Hayashida ◽  
Sigenori Miyamoto ◽  
Shunji Kitamoto ◽  
Hitoshi Negoro ◽  
Hajime Inoue

2009 ◽  
Vol 5 (S267) ◽  
pp. 151-160 ◽  
Author(s):  
Bradley M. Peterson

AbstractWe review briefly direct and indirect methods of measuring the masses of black holes in galactic nuclei, and then focus attention on supermassive black holes in active nuclei, with special attention to results from reverberation mapping and their limitations. We find that the intrinsic scatter in the relationship between the AGN luminosity and the broad-line region size is very small, ~0.11 dex, comparable to the uncertainties in the better reverberation measurements. We also find that the relationship between reverberation-based black hole masses and host-galaxy bulge luminosities also seems to have surprisingly little intrinsic scatter, ~0.17 dex. We note, however, that there are still potential systematics that could affect the overall mass calibration at the level of a factor of a few.


2013 ◽  
Vol 549 ◽  
pp. A119 ◽  
Author(s):  
A. Caccianiga ◽  
R. Fanali ◽  
P. Severgnini ◽  
R. Della Ceca ◽  
E. Marchese ◽  
...  
Keyword(s):  

2012 ◽  
Vol 756 (2) ◽  
pp. 179 ◽  
Author(s):  
Nicholas J. McConnell ◽  
Chung-Pei Ma ◽  
Jeremy D. Murphy ◽  
Karl Gebhardt ◽  
Tod R. Lauer ◽  
...  

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