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| Paper: |
Another approach to the boundary layer in T Tauri stars |
| Volume: |
132, Star Formation with the Infrared Space Observatory (ISO) |
| Page: |
394 |
| Authors: |
Obach, Carsten |
| Abstract: |
For a slightly generalized dynamical viscosity distribution of the standard disk model the dynamical and thermal structure of the boundary layer between an accretion disk and a classical T Tauri star are calculated. Stationary solutions for flux and temperature conditions at the inner boundary using the slim disk approximation with radial radiative and advective energy transport are presented. |
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