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Models of steady thick accretion discs around a Schwarzschild hole*

Published online by Cambridge University Press:  19 July 2016

M. R. Anderson
M. R. Anderson*
Affiliation:
Institute of Astronomy, Cambridge, CB3 0HA, England

Abstract

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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.

Type
IV. Prime Movers, Models and Mechanisms
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 409 - 410
Copyright
Copyright © Reidel 1986 

References

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