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

被引：0

作者：

Gorkavyi, Nick ^{[1
]}

机构：

[1] Sci Syst & Applicat Inc SSAI, 10210 Greenbelt Rd,Suite 600, Lanham, MD 20706 USA

来源：

GALAXIES | 2022年 / 10卷 / 03期

关键词：

galaxies; supermassive black holes; accretion model; rotation of galaxies; Tully-Fisher law; Faber-Jackson relation; M-sigma relation; SPACE ORIENTATION; DARK-MATTER; MASS END; ANISOTROPY; STELLAR; BULGE; MILKY;

D O I：

10.3390/galaxies10030073

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：9

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