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On Illumination Effect in AGN Disks
Published online by Cambridge University Press: 19 July 2016
Extract
We consider illumination effects in a weakly self–gravitating (4πGΣ ∼ Ω2z) outer disk region (R ∼ 1017cm) around a supermassive blackhole of M8 = M/108Msun = 1 with relatively high mass accretion rates (Ṁ25 = Ṁ/1025g/s = 1). (e.g., Shlosman and Begelman 1989, APJ, 341, 685; Shore and White 1982, APJ, 256, 390).
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- Poster Contributions: Disks Structure and Emission
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- Copyright © Kluwer 1994