The Effects of Radial Viscous Forces on the Structure of Accretion Disk Boundary Layers

Details The Effects of Radial Viscous Forces on the Structure of Accretion Disk Boundary Layers The Effects of Radial Viscous Forces on the Structure of Accretion Disk Boundary Layers

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...478..417c&link_type=abstract

Astrophysical Journal v.478, p.417

Astronomy and Astrophysics

Astronomy

7

Comets: General, Ism: Dust, Extinction, Methods: Statistical, Molecular Processes

Scientific paper

We construct steady flow models of the inner disk and boundary layer in
accretion disks, including the radial viscous force. We find that the
radial viscous force has little effect on the thermal boundary layer but
strongly affects the size and structure of the dynamical boundary layer.

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