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Computer Simulation of the Evolution of Active AGN: Single Supermassive Star Versus a Cluster of Massive WR Stars
Published online by Cambridge University Press: 03 August 2017
Abstract
The evolution of gas and stars in galactic nuclei is reconsidered and numerical models of early evolutionary phases of galactic nuclei are discussed, in particular the evolution of a supermassive gaseous object as a hypothetical precursor of a supermassive black hole.
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- Session VIII. Inventory and Distribution
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- Copyright © Kluwer 1991