Chrome Extension
WeChat Mini Program
Use on ChatGLM
VIPCreated with Sketch.

The Cosmogony of Super-Massive Black Holes

W.J. Duschl,P.A. Strittmatter

Journal of physics Conference series（2012）

Cited 3|Views7
No score
Abstract
We summarize our recent results on the evolution of super-massive black holes in the cores of galaxies. Our models are based on the viscous, Eddington-limited evolution of self-gravitating accretion disks. We find that, within this framework, one can explain the growth time scales and the luminosities of individual objects as well as the variation of these quantities for AGN with different black hole masses.
More
Translated text
Key words
Accretion Disk,Accretion Rate,Active Galactic Nucleus,Galactic Center,Eddington Limit
AI Read Science
Must-Reading Tree
Example
Generate MRT to find the research sequence of this paper
Chat Paper
Summary is being generated by the instructions you defined