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

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...

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Main Author: Nick Gorkavyi
Format: Article
Language:English
Published: MDPI AG 2022-05-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/10/3/73
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author Nick Gorkavyi
author_facet Nick Gorkavyi
author_sort Nick Gorkavyi
collection DOAJ
description 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.
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spelling doaj.art-597521f04e494feaa67d1e9b72471c812023-11-23T16:44:14ZengMDPI AGGalaxies2075-44342022-05-011037310.3390/galaxies10030073Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma RelationsNick Gorkavyi0Science Systems and Applications, Inc. (SSAI), 10210 Greenbelt Road, Suite 600, Lanham, MD 20706, USAThe 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.https://www.mdpi.com/2075-4434/10/3/73galaxiessupermassive black holesaccretion modelrotation of galaxiesTully-Fisher lawFaber-Jackson relation
spellingShingle Nick Gorkavyi
Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations
Galaxies
galaxies
supermassive black holes
accretion model
rotation of galaxies
Tully-Fisher law
Faber-Jackson relation
title Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations
title_full Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations
title_fullStr Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations
title_full_unstemmed Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations
title_short Accretion of Galaxies around Supermassive Black Holes and a Theoretical Model of the Tully-Fisher and M-Sigma Relations
title_sort accretion of galaxies around supermassive black holes and a theoretical model of the tully fisher and m sigma relations
topic galaxies
supermassive black holes
accretion model
rotation of galaxies
Tully-Fisher law
Faber-Jackson relation
url https://www.mdpi.com/2075-4434/10/3/73
work_keys_str_mv AT nickgorkavyi accretionofgalaxiesaroundsupermassiveblackholesandatheoreticalmodelofthetullyfisherandmsigmarelations