Vinsamlegast notið þetta auðkenni þegar þið vitnið til verksins eða tengið í það: https://hdl.handle.net/1946/27756
Accretion disks are complex systems which are not yet entirely understood. Here a short overview is given of accretion disk theory, describing the disks, the thin disk approximation to simplify calculations and a description of the alpha-disk model. The Eddington limit and its role in accretion disks is discussed. Newtonian and Pseudo-Newtonian gravitational potentials are introduced and analyzed. Modeling black hole systems is also covered. Finally, observations of four systems possessing black holes are discussed.
Skráarnafn | Stærð | Aðgangur | Lýsing | Skráartegund | |
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Accretion_Disks.pdf | 1.89 MB | Opinn | Heildartexti | Skoða/Opna | |
Eyðublað.pdf | 46.49 kB | Lokaður | Yfirlýsing |