The Photometric Period of the Cataclysmic Variable HV Andromedae
Solar and Stellar Astrophysics
2015-06-03 v1
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.
Keywords
Cite
@article{arxiv.1111.0348,
title = {The Photometric Period of the Cataclysmic Variable HV Andromedae},
author = {Gerald D. Rude and F. A. Ringwald},
journal= {arXiv preprint arXiv:1111.0348},
year = {2015}
}
Comments
7 pages, 3 figures; accepted for publication in New Astronomy