THE QUASI-PERIODIC OSCILLATIONS OF VV PUPPIS

Four AM Her objects are known to exhibit low-amplitude, rapid quasi-pe riodic oscillations (QPOs) in their optical emission. Here, we present high-speed optical photometric observations of the QPO source VV Pup obtained during 1990 January. The observations were made in unfiltered light. We first confirm the results of Larsson (1989) that VV Pup is a strong source of QPOs and that the QPOs are confined to optical maxi mum showing that the QPOs are produced in or near the X-ray-producing shock formed as the accreting plasma merges onto the white dwarf. We t hen show that: (1) variations in the amplitudes of the QPOs over narro w bandwidths, deltanu approximately 0.1 Hz, around the peak of the QPO s, nu(QPO) approximately 0.6-0.7 Hz, are correlated. We also find a su ggestion that the QPO powers at widely separated frequencies are also positively correlated. These results suggest that the QPOs are due to a broad-band process rather than to a narrow-band feature which wander s slowly in frequency space. (2) We isolate strong damped oscillations in several 81.92 s intervals. The pulse profiles are consistent with damped sinusoids. The strongest feature has an amplitude of several pe rcent with frequency v approximately 0.64 Hz and quality Q approximate ly 21, or a coherence Of tau approximately 6.7. VV Pup is the third QP O source to show evidence of strong oscillations of moderate coherence .