We argue that the observed correlations between central black holes masses M_{BH} and galactic bulge velocity dispersions \sigma_e in the form M_{BH}\propto\sigma_e^4 may witness on the pregalactic origin of massive black holes. Primordial black holes would be the centers for growing protogalaxies which experienced multiple mergers with ordinary galaxies. This process is accompanied by the merging of black holes in the galactic nuclei
We study the number and interaction rates of supermassive black holes in galactic bulges as predicte...
This paper presents an analysis of the correlation between the number of globular clusters ($N_{GC}$...
The masses of supermassive black holes correlate almost perfectly with the velocity dispersions of t...
Recent work has demonstrated that there is a tight correlation between the mass of a black hole and ...
Supermassive black holes appear to be uniquely associated with galactic bulges. The mean ratio of bl...
We test the evolution of the correlation between black hole mass and bulge velocity dispersion (MBH-...
We assess models for the assembly of supermassive black holes (SMBHs) at the center of galaxies that...
Recent studies have revealed a strong relation between the sample-averaged black hole (BH) accretion...
We demonstrate a strong correlation between supermassive black hole (SMBH) mass and the global struc...
We analyse the scatter in the correlation between supermassive black hole (SMBH) mass and bulge stel...
In this paper, we examine whether the properties of central black holes in galactic nuclei correlate...
Recent observations by \citet{Ferrarese2006} and \citet{Wehner2006} reveal that a majority of galaxi...
The masses of supermassive black holes (SBHs) show correlations with bulge properties in disk and el...
© 2018 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Socie...
High-dynamic-range surface photometry in a companion paper makes possible accurate measurement of th...
We study the number and interaction rates of supermassive black holes in galactic bulges as predicte...
This paper presents an analysis of the correlation between the number of globular clusters ($N_{GC}$...
The masses of supermassive black holes correlate almost perfectly with the velocity dispersions of t...
Recent work has demonstrated that there is a tight correlation between the mass of a black hole and ...
Supermassive black holes appear to be uniquely associated with galactic bulges. The mean ratio of bl...
We test the evolution of the correlation between black hole mass and bulge velocity dispersion (MBH-...
We assess models for the assembly of supermassive black holes (SMBHs) at the center of galaxies that...
Recent studies have revealed a strong relation between the sample-averaged black hole (BH) accretion...
We demonstrate a strong correlation between supermassive black hole (SMBH) mass and the global struc...
We analyse the scatter in the correlation between supermassive black hole (SMBH) mass and bulge stel...
In this paper, we examine whether the properties of central black holes in galactic nuclei correlate...
Recent observations by \citet{Ferrarese2006} and \citet{Wehner2006} reveal that a majority of galaxi...
The masses of supermassive black holes (SBHs) show correlations with bulge properties in disk and el...
© 2018 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Socie...
High-dynamic-range surface photometry in a companion paper makes possible accurate measurement of th...
We study the number and interaction rates of supermassive black holes in galactic bulges as predicte...
This paper presents an analysis of the correlation between the number of globular clusters ($N_{GC}$...
The masses of supermassive black holes correlate almost perfectly with the velocity dispersions of t...