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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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