There are either a near kinematic distance of 5.5Â kpc or a far distance of 8.8Â kpc for a Galactic supernova remnant ( SNR ) G32.8 - 0.1 derived by using the rotation curve of the Galaxy .
Here we make sure that the remnant distance is the farther one 8.8Â kpc through solving a group of equations for the shell-type remnants separately at the adiabatic-phase and the radiative-phase .
For SNR G346.6 - 0.2 we determine its distance also the farther one 11Â kpc rather than the nearer one 5.5Â kpc .