The Photometric Period of the Cataclysmic Variable HV Andromedae
arXiv:1111.0348 · doi:10.1016/j.newast.2011.11.002
Abstract
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.
7 pages, 3 figures; accepted for publication in New Astronomy