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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| Format: | Article |
| Language: | English |
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MDPI AG
2022-05-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/10/3/73 |