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An international team led by the University of Sydney has identified ASKAP J1745−5051 as the first clear example of a long-period radio transient (LPT) originating in a cataclysmic variable — a closely orbiting pair of stars in which a magnetic white dwarf accretes material from a red dwarf companion.
Observations with CSIRO’s ASKAP radio telescope recorded strongly polarized, repeating radio bursts every ~81 minutes that were accompanied by periodic X‑ray outbursts detected by NASA’s Swift and the Einstein Probe.
Optical spectroscopy from the SOAR telescope confirmed a white dwarf–red dwarf binary with matching orbital period; the radio and X‑ray peaks are offset in phase, indicating different emission regions.
The discovery, published in Nature Astronomy in early June 2026 and led by PhD student Kovi Rose, ties together multiwavelength evidence and offers a template to interpret about a dozen previously puzzling LPTs found across the Milky Way.
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The Conversation - World NewsMysterious signals keep coming from space. We have found their ‘Rosetta stone’Kovi Rose, University of Sydney








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