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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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