The Structure of Accretion Disk Boundary Layers in CVs

Details The Structure of Accretion Disk Boundary Layers in CVs The Structure of Accretion Disk Boundary Layers in CVs

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.2607c&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #26.07; Bulletin of the American Astronomical Society, Vol. 27, p.1324

Astronomy and Astrophysics

Astronomy

Scientific paper

We consider the effects of both bulk viscosity and convective heat transport on the structure of accretion disk boundary layers in CVs. We find that the bulk viscosity has little effect on the thermal boundary layer, but changes the size and structure of the dynamical boundary layer. In addition, bulk viscosity allows one to resolve the radial shock. Convective heat transport significantly broadens the thermal boundary layer.

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