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Models of steady thick accretion discs around a Schwarzschild hole*
Published online by Cambridge University Press: 19 July 2016
Abstract
An outline is given of a project to model thick accretion discs around a black hole. A simple shear viscosity is assumed and the effects of radiation transport and thermal conduction neglected. Preliminary results are given for the equatorial structure of the model discs.
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- IV. Prime Movers, Models and Mechanisms
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- Copyright © Reidel 1986