Simulations identify black hole-giant collisions as the main formation channel for ultracompact black hole-white dwarf binaries in globular clusters, with mock catalogs suggesting order-one LISA-detectable sources in the Milky Way.
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2 Pith papers cite this work. Polarity classification is still indexing.
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New SED fitting of ASKAP J1745-5051 using model atmospheres, corrected photometry, and added NIR data yields a 15,000 K WD plus 0.05 solar-mass sub-stellar donor at ~320 pc, suggesting a period-bouncer CV.
citing papers explorer
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Formation of Black Hole-White Dwarf X-ray Binaries in Globular Clusters
Simulations identify black hole-giant collisions as the main formation channel for ultracompact black hole-white dwarf binaries in globular clusters, with mock catalogs suggesting order-one LISA-detectable sources in the Milky Way.
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The Long-Period Radio Transient and Cataclysmic Variable ASKAP J1745-5051: Evidence for a 15,000 K White Dwarf and a Sub-Stellar Donor
New SED fitting of ASKAP J1745-5051 using model atmospheres, corrected photometry, and added NIR data yields a 15,000 K WD plus 0.05 solar-mass sub-stellar donor at ~320 pc, suggesting a period-bouncer CV.