An international team of astronomers led by Australia's International Centre for Radio Astronomy Research (ICRAR), with the participation of the Institute of Space Sciences (ICE-CSIC), the Institute of Space Studies of Catalonia (IEEC), and the Institute of Astrophysics of Andalusia (IAA-CSIC), has detected a new long-period transient object: a recently discovered type of cosmic phenomenon. The study is published today in the journal Nature.
The object, known as ASKAP J1832-0911, emits pulses of radio waves and X-rays for two minutes every 44 minutes. This is the first time objects like these, called long-period transients (LPTs), have been detected in X-rays. It is located in our Milky Way galaxy, about 15,000 light-years from Earth. Astronomers hope it may provide insights into the sources of similar mysterious signals observed across the sky. Detecting these objects using both X-rays and radio waves may help astronomers find more examples and learn more about them.
The team discovered ASKAP J1832-0911 by using ASKAP radio telescope on Wajarri Country in Australia, owned and operated by Australia’s national science agency, CSIRO. They correlated the radio signals with X-ray pulses detected by NASA’s Chandra X-ray Observatory, which was coincidentally observing the same part of the sky.
“Discovering that ASKAP J1832-0911 was emitting X-rays felt like finding a needle in a haystack,” said lead author Dr Ziteng (Andy) Wang from the Curtin University node of ICRAR.
“The ASKAP radio telescope has a wide field view of the night sky, while Chandra observes only a fraction of it. So, it was fortunate that Chandra observed the same area of the night sky at the same time”, he adds.
A new cosmic phenomenon
LPTs, which emit radio pulses that occur minutes or hours apart, are a relatively recent discovery. Since their first detection by ICRAR researchers in 2022, ten LPTs have been discovered by astronomers across the world. Currently, there is no clear explanation for what causes these signals, or why they ‘switch on’ and ‘switch off’ at such long, regular and unusual intervals.
“This object is unlike anything we have seen before. ASKAP J1831-0911 could be a magnetar (the core of a dead star with powerful magnetic fields), or it could be a pair of stars in a binary system where one of the two is a highly magnetised white dwarf (a low-mass star at the end of its evolution)”, Dr Wang said.
“However, even those theories do not fully explain what we are observing. This discovery could indicate a new type of physics or new models of stellar evolution”, he adds.
According to second author Professor Nanda Rea, researcher at the ICE-CSIC and IEEC, “finding one such object hints at the existence of many more. The discovery of its transient X-ray emission opens fresh insights into their mysterious nature.”
“What was also truly remarkable is that this study showcases an incredible teamwork effort, with contributions from researchers across the globe with different and complementary expertise,” added Rea, who contributed to the results interpretation and the X-band observations.
“This is the first time that X-ray emission has been detected in this kind of object, and the most surprising thing is that its behavior is unlike anything known in our galaxy: it is extremely bright, varies greatly in intensity and does not fit into traditional categories, such as neutron stars or white dwarfs,” says Miguel A. Pérez-Torres, an IAA-CSIC researcher involved in the study.
“The object is thousands of times more luminous than expected based on its rotation, which forces us to reconsider some physical models,” notes Miguel A. Pérez-Torres (IAA-CSIC). “It could be an aging magnetar—a neutron star with an extremely strong magnetic field—or a supermagnetized white dwarf. Both options challenge current theories.”
The discovery also helps narrow down what the objects might be. Since X-rays are much higher energy than radio waves, any theory must account for both types of emissions – a valuable clue, given their nature remains a cosmic mystery.
