Expanding motion in the ionized envelope of HBV 475

Expansion velocities in the ionized envelope of HBV 475 are obtained from line profiles of H-alpha, He I 6678, 7065, and forbidden Fe VII 6087. Two components of forbidden Fe VII 6087 show evidence of outward gas motion with high velocities from the central star. H-alpha and He I 6678 profiles are very similar to those obtained from observations of forbidden O III and Ne III lines, and have gas motion velocities corresponding to full widths at half-maximum of the lines which do not exceed the velocities of Fe(+6). Through investigations of He(+) and Fe(+5) ionization structures, it is concluded that the interacting stellar winds model is favorable to explain the velocity fields suggested by the line profiles