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Stochastic Correlation Model of Galactic Bulge Velocity Dispersions and Central Black Holes Masses

V. I. Dokuchaev·Yu. N. Eroshenko
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Abstract

We consider the cosmological model in which a part of the Universe Ω_h\sim 10^-5 is in the form of primordial black holes with mass \sim 10^5M_\odot. These primordial black holes would be centers for growing protogalaxies which experienced multiple mergers with ordinary galaxies. This process of galaxies formation is accompanied by the merging of central black holes in the galactic nuclei. It is shown that recently discovered correlations between the central black holes and bulges of galaxies are naturally reproduced in this scenario.

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V. I. Dokuchaev, Yu. N. Eroshenko. 2002-02-01. Stochastic Correlation Model of Galactic Bulge Velocity Dispersions and Central Black Holes Masses. https://doi.org/10.1134/1.1424357

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