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The Photometric Period of the Cataclysmic Variable HV Andromedae

We present four nights of time-resolved photometry of the cataclysmic variable star HV And. Our time series analysis has revealed a prominent period at 3.368 +/- 0.060 hours, as well as some low frequency power. We interpret this signal, from saw-tooth waves in the light curve, as evidence of superhumps in HV And.

preprint2011arXivOpen access
Gerald D. Rude IIF. A. Ringwald
astro-ph.SR
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Open access2 authors1 topic
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Gerald D. Rude IIF. A. Ringwald

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