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KUV 01584-0939: A Helium-transferring Cataclysmic Variable with an Orbital Period of 10 Minutes

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arxiv astro-ph/0201191 v1 pith:VADH4CTX submitted 2002-01-12 astro-ph

Brian Warner (Univ. of Cape Town) , Patrick A. Woudt (Univ. of Cape Town) This is my paper · ORCID
classification astro-ph
keywords periodorbitalaliascasecataclysmiccet3combinedhelium-transferring
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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.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A survey of ultra-compact high-state AM CVn binaries with ZTF and Gaia: New discoveries and observational constraints on Galactic space density

    astro-ph.SR 2026-08 conditional novelty 7.0 of 10

    Three new high-state AM CVn binaries are discovered, giving a local space density of about 1 to 3 per 10^8 cubic parsecs and LISA detection estimates near 36% of the Galactic population.

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