Abstract
We consider a cosmological model in which part of the Universe, Ωh∼10−5, is in the form of primordial black holes with masses of ∼ 105 M ⊙. These primordial black holes were the centers for growing protogalaxies, which experienced multiple mergers with ordinary galaxies and with each other. The galaxy formation is accompanied by the merging and growth of central black holes in the galactic nuclei. We show that the recently discovered correlations between central black hole masses and galactic bulge parameters naturally arise in this scenario.
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Translated from Pis’ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, Vol. 27, No. 12, 2001, pp. 883–889.
Original Russian Text Copyright © 2001 by Dokuchaev, Eroshenko.
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Dokuchaev, V.I., Eroshenko, Y.N. A stochastic model for correlations between central black hole masses and galactic bulge velocity dispersions. Astron. Lett. 27, 759–764 (2001). https://doi.org/10.1134/1.1424357
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DOI: https://doi.org/10.1134/1.1424357