We present fast photometric observations of KR Aurigae, a nova-like va
riable, made during 1984-1988, in the B and U bands. The light curves
show large-amplitude pulsations with periods in the range 480-780 s. T
he period is found to be different even on consecutive nights and, the
refore, these pulsations are interpreted as ''quasi-periodic'' in natu
re. The pulsation periods in the bright state are positively correlate
d with the source intensity, but the low-state periods do not follow t
his linear trend. We discuss possible explanations of the quasi-period
ic oscillations. Pulsations with period in the 1050-1600 s range are a
lso found in the data, which can be attributed to broader features see
n in the light curves. We also present the X-ray results from analysis
of the observations made with the Einstein Observatory. The X-ray spe
ctrum is found to be soft with a large hydrogen column density.