Abstract: 
In the simulation of a protoplanetary disc with a power law density profile, a disc instability is detected. The instability arises only with a power law profile and is affected by the power index. Thus, the impact of initial density profile is large within the employed numerical model.
Keywords: 
Issue
Pages: 
63-68
File: 
  
  
 snytnikov_1.pdf
 (193.21 KB)
