We present simultaneous X-ray ( \lambda _ { peak } \sim 44 { \AA } ) and EUV ( \lambda _ { peak } = 89 { \AA } ) light curves for the magnetic cataclysmic variable QQ Vulpeculae , obtained with the EUVE satellite . We find that the unique shape of the X-ray light curve is different from previously obtained X-ray light curves of QQ Vul and provides evidence for two-pole accretion . Detailed examination of the photometric data indicates that QQ Vul undergoes a stellar eclipse of the X-ray emitting region , indicative of a high binary inclination . We discuss possible implications for the nature of this system given the observed shape of its EUV and X-ray light curves .