| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1779289 | New Astronomy | 2012 | 4 Pages |
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 h, 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.
► We present four nights of time-resolved photometry of the cataclysmic variable star HV And. ► We find a period at 3.368 ± 0.060 h, as well as some low frequency power. ► We interpret this signal as superhumps in HV And.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Gerald D. Rude II, F.A. Ringwald,