  We have obtained time series optical spectra of the cataclysmic variable PQ
And in quiescence. The spectra show a white dwarf continuum with narrow Balmer
emission superimposed over strong Balmer absorption. The emission lines have
blue and red components whose strength changes with time. An analysis of the
H$\alpha$ emission line implies a short orbital period below the period gap.
Given its lack of accretion disk features, its large and infrequent outbursts,
and an orbital period below the period gap, PQ And is probably a low accretion
rate object similar to WZ Sge. In addition, white dwarf model fits imply that
PQ And is an excellent ZZ Cet candidate.
