On disk accretion

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1983 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 90, pages 79-107 (issn: 0004-640X, eissn: 1572-946X,

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Authors: Urpin, V. A.;

doi: 10.1007/bf00651550

On disk accretion

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Abstract

A simple but sufficiently accurate method for calculating an accretion disk structure is developed. The detailed analysis of the accretion disk is fulfilled by using this method. The effect of turbulent heat transfer on the disk structure is taken into account along with the effect of radiative transfer.

Related Organizations

Russian Academy of Sciences
Russian Federation
National Academy of Sciences of Belarus
Belarus
Physical Technical Institute
Belarus

Keywords

accretion disk structure, Stability and instability of geophysical and astrophysical flows, radiative transfer, Radiative transfer in astronomy and astrophysics, effect of turbulent heat transfer, Galactic and stellar dynamics

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