Origin of Correlations between Central Black Holes Masses and Galactic Bulge Velocity Dispersions

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dc.creatorDokuchaev, V. I.
dc.creatorEroshenko, Yu. N.
dc.date2002-09-17
dc.date.accessioned2026-07-07T11:46:02Z
dc.date.available2026-07-07T11:46:02Z
dc.descriptionWe argue that the observed correlations between central black holes masses M_{BH} and galactic bulge velocity dispersions σ_e in the form M_{BH}\proptoσ_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.
dc.description6 pages, 1 figure, submitted to Astron. and Astrophys. Transactions
dc.identifierhttps://arxiv.org/abs/astro-ph/0209324
dc.identifierhttp://arxiv.org/abs/astro-ph/0209324
dc.identifierAstron.Astrophys.Trans.22:727,2003
dc.identifierdoi:10.1080/10556790310001609115
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202084
dc.subjectAstrophysics
dc.titleOrigin of Correlations between Central Black Holes Masses and Galactic Bulge Velocity Dispersions
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