An international team of astronomers led by scientists from the Netherlands has shown that a white dwarf and a red dwarf orbiting each other every two hours are emitting radio pulses. Thanks to observations with several telescopes, the researchers were able to determine the origin of these pulses with certainty for the first time. Their results are published in Nature Astronomy.
In recent years, thanks to better analysis techniques, researchers have detected radio pulses that last from seconds to minutes and seem to come from stars in the Milky Way. There have been many hypotheses about what triggers these pulses, but until now there has been no hard evidence. An international study led by Iris de Ruiter of the Netherlands changes this.
De Ruiter, who received her Ph.D. from the University of Amsterdam in October 2024, is now a postdoctoral researcher at the University of Sydney (Australia). During the last year of her Ph.D., she developed a method to search for radio pulses of seconds to minutes in the LOFAR archive. While improving the method, she discovered a single pulse in the 2015 observations. When she subsequently sifted through more archive data from the same patch of sky, she discovered six more pulses. All the pulses came from a source called ILTJ1101.