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On Illumination Effect in AGN Disks

Published online by Cambridge University Press:  19 July 2016

Insu Yi
Insu Yi*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden St., Cambridge, MA 02138, USA

Extract

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We consider illumination effects in a weakly self–gravitating (4πGΣ ∼ Ω2 z) outer disk region (R ∼ 1017cm) around a supermassive blackhole of M 8 = M/108Msun = 1 with relatively high mass accretion rates (Ṁ 25 = Ṁ/1025g/s = 1). (e.g., Shlosman and Begelman 1989, APJ, 341, 685; Shore and White 1982, APJ, 256, 390).

Type
Poster Contributions: Disks Structure and Emission
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 493
Copyright
Copyright © Kluwer 1994