| Autor: |
Kai, Takashi, Baba, Tamon, Arai, Kenzo, Fujimoto, Shin-ichiro |
| Jazyk: |
angličtina |
| Rok vydání: |
2010 |
| Předmět: |
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| Zdroj: |
Physics Reports of Kumamoto University. 13(2):163-170 |
| ISSN: |
0303-4070 |
| Popis: |
We investigate the difference between the accretion disk models based on two kinds of α-prescription of viscosity. The models are constructed with self-gravity in the vertical direction of the disk around a supermassive black hole. It is found that the structures are completely different in the self-gravity dominant region, though they are almost the same for the standard disk model. We should be careful in treating viscosity, if self-gravity is taken into account for a disk model of an emitting region of H2O masers in an active galactic nucleus(AGN). |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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