ASPCS
 
Back to Volume
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.
Back to Volume