The eclipsing cataclysmic variable GS Pavonis: Evidence for disk radius changes

We have obtained differential time series photometry of the cataclysmic var iable GS Pavonis over a timespan of 2 years. These show that this system is deeply eclipsing (similar to 23.5 mag) with an orbital period of 3.72 hr. The eclipse depth and out-of-eclipse light levels are correlated. From this correlation we deduce that the disk radius is changing and that the eclips es in the low state are total. The derived distance to GS Pav is 790+/-90 p c, with a height above the galactic plane of 420+/-60 pc. We classify GS Pa v as a novalike system.