Student Astronomer Discovers ‘Rosetta Stone’ For Mysterious Cosmic Signals
These are antennas of CSIRO's Australian SKA Pathfinder with the Milky Way overhead. Credit: Alex Cherney/CSIRO
June 2, 2026
By Eurasia Review
An international team led by astronomers at the University of Sydney has uncovered the clearest evidence yet for the origin of an unusual class of cosmic signals. In doing so, they have identified a rare stellar system that is providing scientists with a natural laboratory to study extreme physics.
Using CSIRO’s ASKAP radio telescope, the team discovered a small, dense star, called a white dwarf, shredding material from its larger, but less dense, companion star.
As this material spirals in, it produces powerful bursts of radio waves and X-rays in a cycle that repeats every 1.4 hours.
The findings are published in Nature Astronomy.
Lead author and PhD student Kovi Rose from the University of Sydney’s School of Physics and CSIRO said this provides the first confirmed identification of a what astronomers call ‘long-period radio transients’: cosmic pulses discovered from just a few remote regions of our galaxy.
“For the first time we have pinpointed the origin of these signals, confirming the source to be a ‘cataclysmic variable’, or an accreting white dwarf star,” said Mr Rose.
“Long-period radio transients have puzzled astronomers for years,” Mr Rose said. “We’ve only found about a dozen, and their origins have been unclear. Now, we’ve been able to show that the source for one of these transients comes from a white dwarf actively pulling material from a companion star.”
A rare and revealing system
The newly identified system, named ASKAP J1745−5051, consists of a white dwarf – a dense stellar remnant roughly the size of Earth but with the mass close to that of the Sun – paired with a larger but lower-mass red dwarf star of about one-tenth the Sun’s mass. The two stars orbit each other extremely closely, completing a full orbit in just over an hour.
As material from the less massive star is drawn towards the white dwarf, it heats up and emits X-rays. At the same time, interactions between the stars’ magnetic fields generate regular radio bursts, meaning the signal occurs at specific intervals.
“These emissions are all tied to the orbital motion of the system,” Mr Rose said. “But interestingly, the radio and X-ray signals don’t peak at the same time, which tells us they’re being produced in different regions of the system.”
The team found that the radio emission likely originates where the magnetic fields of the two stars meet and interact with the charged material being ripped from the companion star, producing tightly beamed bursts of radiation.
Solving a cosmic mystery
Long-period radio transients were initially thought to be slow-spinning neutron stars, known as pulsars. However, current models suggest neutron stars rotating this slowly should not be able to produce such signals.
The new discovery strengthens an alternative explanation: that at least some of these mysterious bursts come from systems of two stars, involving white dwarfs.
“Some similar objects had been linked to binary systems before, but this is the first one where we can clearly see both stars and the accretion process in action,” said Professor Murphy, Head of School at the University of Sydney School of Physics and Chief Investigator at the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).
The system is also only the second known long-period radio transient to emit regular X-rays – and the first where the cause of the regularity has been confirmed.
A ‘Rosetta stone’ for future discoveries
This unique system was discovered using the ASKAP radio telescope, owned and operated by CSIRO, Australia’s national science agency. ASKAP’s mix of coverage, resolution, and sensitivity is unparalleled in radio astronomy, allowing for such unusual signals to be detected that would otherwise be missed.
The researchers say that ASKAP J1745-5051 could act as a reference point for understanding other long-period radio transients.
“This system gives us a way to decode these signals. It could help us determine whether other long-period transients are more like pulsars or like white dwarf systems, acting like a stellar Rosetta stone,” said Mr Rose, referring to the archaeological object discovered in Egypt that helped translate ancient hieroglyphics.
The discovery also provides a unique opportunity to study extreme plasma physics and magnetic interactions under conditions that cannot be replicated on Earth.
“These systems are natural laboratories,” Mr Rose said. “They allow us to test our understanding of how matter behaves in strong magnetic fields and under intense gravitational forces.”
Future research
The team plans further observations combining radio, optical and X-ray telescopes to better understand how these emissions are generated and whether similar mechanisms can explain the full population of long-period radio transients.
“Each new discovery is helping us piece together the bigger picture,” Mr Rose said. “We’re only just beginning to understand this new class of cosmic events.”
The international team included astronomers from the United States, China, Canada, Spain, Israel and Australia. The team used CSIRO’s Australia Telescope Compact Array and ASKAP radio telescopes in Australia, the MeerKAT radio telescope in South Africa, the SOAR and Magellan optical telescopes in Chile, and the space-based Swift (UV/X-ray) and Einstein Probe (X-ray) telescopes.
Student astronomer discovers ‘Rosetta stone’ for mysterious cosmic signals
White dwarf binary provides unique natural laboratory for extreme physics
image:
Artists’ impression of the white dwarf binary ASKAP J1745-5051. The smaller, dense white dwarf star is accreting material from the larger, but less dense red dwarf star. The interaction of their magnetic fields and the heat from the material accretion creates signals in radio and X-ray light frequencies.
view moreCredit: Credit: Carl Knox (OzGrav/Swinburne) and Dr Joshua Preston Pritchard (CSIRO).
An international team led by astronomers at the University of Sydney has uncovered the clearest evidence yet for the origin of an unusual class of cosmic signals. In doing so, they have identified a rare stellar system that is providing scientists with a natural laboratory to study extreme physics.
Using CSIRO’s ASKAP radio telescope, the team discovered a small, dense star, called a white dwarf, shredding material from its larger, but less dense, companion star.
As this material spirals in, it produces powerful bursts of radio waves and X-rays in a cycle that repeats every 1.4 hours.
The findings are published in Nature Astronomy.
Lead author and PhD student Kovi Rose from the University of Sydney’s School of Physics and CSIRO said this provides the first confirmed identification of a what astronomers call ‘long-period radio transients’: cosmic pulses discovered from just a few remote regions of our galaxy.
“For the first time we have pinpointed the origin of these signals, confirming the source to be a ‘cataclysmic variable’, or an accreting white dwarf star,” said Mr Rose.
“Long-period radio transients have puzzled astronomers for years,” Mr Rose said. “We’ve only found about a dozen, and their origins have been unclear. Now, we’ve been able to show that the source for one of these transients comes from a white dwarf actively pulling material from a companion star.”
A rare and revealing system
The newly identified system, named ASKAP J1745−5051, consists of a white dwarf – a dense stellar remnant roughly the size of Earth but with the mass close to that of the Sun – paired with a larger but lower-mass red dwarf star of about one-tenth the Sun’s mass. The two stars orbit each other extremely closely, completing a full orbit in just over an hour.
As material from the less massive star is drawn towards the white dwarf, it heats up and emits X-rays. At the same time, interactions between the stars’ magnetic fields generate regular radio bursts, meaning the signal occurs at specific intervals.
“These emissions are all tied to the orbital motion of the system,” Mr Rose said. “But interestingly, the radio and X-ray signals don’t peak at the same time, which tells us they’re being produced in different regions of the system.”
The team found that the radio emission likely originates where the magnetic fields of the two stars meet and interact with the charged material being ripped from the companion star, producing tightly beamed bursts of radiation.
Solving a cosmic mystery
Long-period radio transients were initially thought to be slow-spinning neutron stars, known as pulsars. However, current models suggest neutron stars rotating this slowly should not be able to produce such signals.
The new discovery strengthens an alternative explanation: that at least some of these mysterious bursts come from systems of two stars, involving white dwarfs.
“Some similar objects had been linked to binary systems before, but this is the first one where we can clearly see both stars and the accretion process in action,” said Professor Murphy, Head of School at the University of Sydney School of Physics and Chief Investigator at the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).
The system is also only the second known long-period radio transient to emit regular X-rays – and the first where the cause of the regularity has been confirmed.
A ‘Rosetta stone’ for future discoveries
This unique system was discovered using the ASKAP radio telescope, owned and operated by CSIRO, Australia's national science agency. ASKAP’s mix of coverage, resolution, and sensitivity is unparalleled in radio astronomy, allowing for such unusual signals to be detected that would otherwise be missed.
The researchers say that ASKAP J1745-5051 could act as a reference point for understanding other long-period radio transients.
“This system gives us a way to decode these signals. It could help us determine whether other long-period transients are more like pulsars or like white dwarf systems, acting like a stellar Rosetta stone,” said Mr Rose, referring to the archaeological object discovered in Egypt that helped translate ancient hieroglyphics.
The discovery also provides a unique opportunity to study extreme plasma physics and magnetic interactions under conditions that cannot be replicated on Earth.
“These systems are natural laboratories,” Mr Rose said. “They allow us to test our understanding of how matter behaves in strong magnetic fields and under intense gravitational forces.”
Future research
The team plans further observations combining radio, optical and X-ray telescopes to better understand how these emissions are generated and whether similar mechanisms can explain the full population of long-period radio transients.
“Each new discovery is helping us piece together the bigger picture,” Mr Rose said. “We’re only just beginning to understand this new class of cosmic events.”
The international team included astronomers from the United States, China, Canada, Spain, Israel and Australia. The team used CSIRO’s Australia Telescope Compact Array and ASKAP radio telescopes in Australia, the MeerKAT radio telescope in South Africa, the SOAR and Magellan optical telescopes in Chile, and the space-based Swift (UV/X-ray) and Einstein Probe (X-ray) telescopes.
DOWNLOAD photos, animations, illustrations and the research paper at this link.
RESEARCH
Rose, K. et al ‘Periodic radio and X-ray emission from an accreting white dwarf binary’ (Nature Astronomy 2026). DOI: 10.1038/s41550-026-02882-x
DECLARATION
The authors declare no competing interests. Research was funded by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), NASA, the Alfred P. Sloan Foundation, the Professor Harry Messel Research Fellowship in Physics Endowment, European Research Council and the China Scholarship Council.
Lead author Kovi Rose from the School of Physics at the University of Sydney, stands in front of an image visualisation of the white dwarf binary ASKAP J1745-5051. Photo: Dr Kirsten Banks (OzGrav).
Credit
Photo: Dr Kirsten Banks (OzGrav). Visual: Carl Knox (OzGrav)
The ASKAP radio telescope at Inyarrimanha Ilgari Bundara, the CSIRO Murchison Radio-astronomy Observatory on Wajarri Yamaji Country in Western Australia.
Credit
Credit: Alex Cherney/CSIRO
Journal
Nature Astronomy
Method of Research
Observational study
Subject of Research
Not applicable
Article Title
Periodic radio and X-ray emission from an accreting white dwarf binary
Article Publication Date
1-Jun-2026
UNC-Chapel Hill astronomers help crack cosmic radio mystery
image:
Artist’s impression of the white dwarf binary ASKAP J1745-5051. The smaller, dense white dwarf star is accreting material from the larger, but less dense red dwarf star. The interaction of their magnetic fields and the heat from the material accretion creates signals in radio and X-ray light frequencies. Credit: Carl Knox (OzGrav/Swinburne) and Dr. Joshua Preston Pritchard (CSIRO).
view moreCredit: Credit: Carl Knox (OzGrav/Swinburne) and Dr. Joshua Preston Pritchard (CSIRO).
A small, dense dead star caught tearing material from a companion star has helped astronomers solve one of the universe’s most perplexing mysteries and researchers at UNC-Chapel Hill played a key role in uncovering the answer.
Working as part of an international collaboration, Carolina astronomers Dr. Igor Andreoni, Dr. Brad Barlow and doctoral student Jonathan Carney helped identify the source of a mysterious class of cosmic signals known as long-period radio transients. The findings, published in Nature Astronomy, provide some of the strongest evidence yet for the origin of these unusual bursts of radio waves, which can repeat over periods ranging from minutes to hours and have puzzled astronomers since their discovery.
The breakthrough began when researchers led by graduate student Kovi Rose at the University of Sydney used the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope to detect powerful bursts of radio waves repeating every 1.4 hours. The observations with multiple telescopes suggested the signals were coming from a binary star system containing a white dwarf, a dense stellar remnant roughly the size of Earth but with a mass comparable to the Sun, and a low-mass red dwarf companion.
To test the idea, the Carolina team quickly secured observing time on the 4.1-meter Southern Astrophysical Research (SOAR) Telescope in Chile.
“The SOAR observations were essential to the success of this project,” said Andreoni, assistant professor in the department of physics and astronomy at UNC-Chapel Hill. “Our data revealed that we were looking at two stars orbiting each other and we could measure the rotation period.”
Late-night observations conducted by Andreoni, Barlow and Carney revealed telltale signatures in the system’s light that confirmed the presence of a magnetic cataclysmic variable — a binary system in which a white dwarf pulls material from a companion star. As that material spirals toward the white dwarf, it heats to extreme temperatures, producing distinctive optical and X-ray emissions.
“The atmosphere in the observing room that night was electric,” said Barlow, associate professor in the department of physics and astronomy at UNC-Chapel Hill. “As soon as the spectrum came up on the screen, those unmistakable emission lines told us we had something special on our hands. It’s not often you get to play a role in discoveries of this magnitude.”
The system, designated ASKAP J1745−5051, consists of a white dwarf and a red dwarf star with about one-tenth the Sun’s mass. The stars orbit each other so closely that they complete a full orbit in just over an hour. While material is stripped from the red dwarf and collected onto the white dwarf, interactions between the stars’ powerful magnetic fields generate regular radio bursts that can be detected across vast distances in space.
“The resolution and sensitivity of the SOAR telescope instrumentation were key,” said Carney, a graduate student in the department of physics and astronomy at UNC-Chapel Hill. "The observations were made possible in part by the Goodman spectrograph, a Carolina-designed instrument mounted on the SOAR Telescope in Chile. UNC originally initiated the SOAR Telescope project in 1987 to expand access to the southern sky for students and researchers."
The discovery may finally explain the origin of some long-period radio transients. When astronomers first detected these signals, many suspected they came from unusually slow-spinning neutron stars known as pulsars. Existing theories suggest neutron stars rotating this slowly should not be capable of producing such emissions. The new findings strengthen an alternative explanation: that some of these mysterious signals are generated by interacting binary star systems involving white dwarfs.
Researchers say ASKAP J1745−5051 could serve as a crucial guide for interpreting future discoveries. Much like the Rosetta Stone helped scholars decipher ancient Egyptian hieroglyphics, this system may provide astronomers with a reference point for determining whether newly discovered long-period radio transients originate from pulsars, white dwarf binaries or other exotic objects.
Beyond solving a longstanding astronomical puzzle, the system offers scientists a rare opportunity to study extreme magnetic fields, high-energy plasma and the behavior of matter under conditions that cannot be reproduced in laboratories.
The study is available online in the journal Nature Astronomy at: https://www.nature.com/articles/s41550-026-02882-x
Journal
Nature Astronomy
Article Title
Periodic radio and X-ray emission from an accreting white dwarf binary
Article Publication Date
1-Jun-2026






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