2022
DOI: 10.3390/galaxies10030073
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Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations

Abstract: The observed Tully-Fisher and Faber-Jackson laws between the baryonic mass of galaxies and the velocity of motion of stars at the edge of galaxies are explained within the framework of the model of accretion of galaxies around supermassive black holes (SMBH). The accretion model can also explain the M-sigma relation between the mass of a supermassive black hole and the velocity of stars in the bulge. The difference in the mechanisms of origin of elliptical galaxies with low angular momentum and disk galaxies w… Show more

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Cited by 1 publication
(2 citation statements)
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“…The Big Bang scatters black holes that did not enter the Big Hole throughout the Universe. In this process, supermassive black holes (SMBH) surviving the maximum compression can serve as seeds for the formation of galaxies [21].…”
Section: Methodsmentioning
confidence: 99%
See 1 more Smart Citation
“…The Big Bang scatters black holes that did not enter the Big Hole throughout the Universe. In this process, supermassive black holes (SMBH) surviving the maximum compression can serve as seeds for the formation of galaxies [21].…”
Section: Methodsmentioning
confidence: 99%
“…After the discovery of gravitational waves generated by the merger of stellar-mass black holes (Abbott et al [16]), hypotheses emerged suggesting that all dark matter consists of black holes (Kashlinsky [17]; Bird et al [18]; Clesse and Garcia-Bellido [19]). Given that supermassive black holes are found at the center of every galaxy [20,21], one can assert the exceptional importance of black holes for cosmological models. Note the article by Di Valentino et al [22] about non-zero curvature of space, supporting the idea of a closed universe or a universe inside a black hole.…”
Section: Introductionmentioning
confidence: 99%