H i channel maps of the MCSNR J0527−7104 region. The dimensions of the SNR determined in KSP13 are shown by the green ellipse in each panel. The red dashed line indicates the approximate position of the giant H i shell GS 70 (Kim et al. 1999) associated with the N 206 star forming region. The heliocentric velocities are also given. In the 226 km s^-1, 231 km s^-1, 236 km s^-1, and 241 km s^-1panels there is a noticeable reduction in H i density to the northwest of the shell.