Gasdynamic features of detached shells around carbon stars with variable ma
ss loss rate are investigated in detail numerically. It is shown that a she
ll is unstable and also, 2D perturbations are less developed that 3D ones.
The structure of perturbed flows corresponding to different evolution scena
rios is compared. The results obtained seem to be promising for interpretat
ion of observations, in particular, the recently obtained detailed data of
TT Cyg.