High speed photometry of KUV 01584-0939 (alias Cet3) shows that is has a period of 620.26 s. Combined with its hydrogen-deficient spectrum, this implies that it is an AM CVn star. The optical modulation is probably a superhump, in which case the orbital period will be slightly shorter than what we have observed.
CITATION STYLE
Warner, B., & Woudt, P. A. (2002). KUV 01584−0939: A Helium‐transferring Cataclysmic Variable with an Orbital Period of 10 Minutes. Publications of the Astronomical Society of the Pacific, 114(792), 129–131. https://doi.org/10.1086/338621
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