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Article

Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations

Science Systems and Applications, Inc. (SSAI), 10210 Greenbelt Road, Suite 600, Lanham, MD 20706, USA
Academic Editors: Bobomurat Ahmedov, Wenbiao Han and Ahmadjon Abdujabbarov
Galaxies 2022, 10(3), 73; https://doi.org/10.3390/galaxies10030073
Received: 27 March 2022 / Revised: 15 May 2022 / Accepted: 25 May 2022 / Published: 27 May 2022
(This article belongs to the Special Issue Particles and Fields in Black Hole Environment)
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 with high angular momentum can be associated with 3D and 2D accretion. View Full-Text
Keywords: galaxies; supermassive black holes; accretion model; rotation of galaxies; Tully-Fisher law; Faber-Jackson relation; M-sigma relation galaxies; supermassive black holes; accretion model; rotation of galaxies; Tully-Fisher law; Faber-Jackson relation; M-sigma relation
MDPI and ACS Style

Gorkavyi, N. Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations. Galaxies 2022, 10, 73. https://doi.org/10.3390/galaxies10030073

AMA Style

Gorkavyi N. Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations. Galaxies. 2022; 10(3):73. https://doi.org/10.3390/galaxies10030073

Chicago/Turabian Style

Gorkavyi, Nick. 2022. "Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations" Galaxies 10, no. 3: 73. https://doi.org/10.3390/galaxies10030073

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