Implications from the Shape of the Viscosity / Surface Density Relation

Details Implications from the Shape of the Viscosity / Surface Density Relation Implications from the Shape of the Viscosity / Surface Density Relation

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..327m&link_type=abstract

Astrophysics and Space Science, Volume 130, Issue 1-2, pp. 327-330

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Results of new vertical structure computations for cool, convective accretion disks are presented. The influence of the uncertainty in the low temperature opacities on the cool branch of the viscosity-surface density relation is investigated. The author discusses how the shape of this relation allows a prediction of temperatures in the accretion disk during the onset of an outburst and compares this with observations of VW Hydri by Hassall (1984).

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