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A Catalogue of Ultracompact Mass-Transferring White Dwarf Binaries

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arxiv 2505.10535 v1 pith:CIKUQZJD submitted 2025-05-15 astro-ph.SR astro-ph.GAastro-ph.HE

classification astro-ph.SRastro-ph.GAastro-ph.HE
keywords cataloguebinariesknownmass-transferringoverviewultracompactbinarycvn-type
verification ladder T0 review T1 audit T2 compute T3 formal
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We present an overview and catalogue of all known mass-transferring binary systems that have white dwarf accretors and orbital periods shorter than 70 minutes, including the AM CVn-type binary systems and a number of related objects. In this paper, we provide an overview of the literature background and describe recent breakthroughs, open questions, and connections to other fields. This overview is intended to provide a starting point for researchers who are relatively new to the fields of ultracompact binaries or AM CVn-type binaries. We define the scope of the catalogue (the criteria for inclusion) and describe its format and contents (what data have been included for each target). We also summarise the observed properties of the known mass-transferring ultracompact binaries, including their orbital periods and component stellar masses and radii. The catalogue presented here aims to provide a central resource to enable researchers to track the current status of the known sample. At the time of writing, the catalogue includes 123 confirmed binaries and 29 candidates. The catalogue is hosted on a public platform (Zenodo) with version control, and will be updated regularly.

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Cited by 4 Pith papers

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.

  2. Optical Spectroscopy of the Most Compact Accreting Binary Harboring a Magnetic White Dwarf and a Hydrogen-rich Donor

    astro-ph.SR 2025-08 conditional novelty 7.0 of 10

    Gaia19bxc is the first strongly magnetic cataclysmic variable (polar) found below the ~80 minute minimum orbital period, likely powered by a metal-poor donor.

  3. Cataclysmic Variables Photometric Periods from TESS

    astro-ph.SR 2026-07 conditional novelty 6.5 of 10

    TESS photometry yields coherent periods for 1,362 CVs, including roughly 465–565 first determinations, and confirms the 2–3 h period gap with a median period near 3.68 h.

  4. SRG/eROSITA X-ray selected cataclysmic variable candidates observed in SDSS-V DR20

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    eROSITA-selected SDSS-V DR20 spectroscopy yields 587 cataclysmic variables (274 known), including new nearby systems, AM CVns, and a low-accretion-rate polar.

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