I examine the hypothesis that many of the high velocity white dwarfs observed by Oppenheimer et al. (2001) are the remnants of donor stars from binaries that produced type Ia supernovae via the ‘single degenerate’ channel. If this channel is a significant contributor to the Galactic SN Ia supernova rate, then the local density of such remnants with V⊥ > 100 km.s −1 could be as high as 2×10pc, c...