Same as Fig. 14 but for a range of velocity channels of CO emission emerging from a CSE representative of CW Leo. Here, the symmetry axis of the molecules was chosen to be along the magnetic field, which is assumed as a toroidal field with position angle = 125° and inclination 45°. The simulated data has been convolved with the synthesised beam from the observations. The panels are labelled with the velocity with respect to the stellar velocity.