We present Doppler images of the precataclysmic variable V471 Tau. The
se images show a large high-latitude spot similar to other magneticall
y active stars (RS CVn, FK Com), as well as a persistent spot in the d
irection of the white dwarf. Comparison with simultaneous photometry i
s complicated by limited phase coverage, but the spectroscopy and phot
ometry are consistent with each other. The rotational velocity of the
late-type star is 91+/-4 km/s, which implies a star oversized for its
spectral type. (C) 1995 American Astronomical Society.