On May 24, four European telescopes took part in the global effort to understand mysterious cosmic flashes. The telescopes captured flashes of radio waves from an extreme, magnetised star in our galaxy.
Published by the editorial team, 16 November 2020
By studying the site of a spectacular stellar explosion seen in April 2020, a Chalmers-led team of scientists have used four European radio telescopes to confirm that astronomy’s most exciting puzzle is about to be solved. Fast radio bursts, unpredictable millisecond-long radio signals seen at huge distances across the universe, are generated by extreme stars called magnetars – and are astonishingly diverse in brightness.
For over a decade, the phenomenon known as fast radio bursts has excited and mystified astronomers. These extraordinarily bright but extremely brief flashes of radio waves – lasting only milliseconds – reach Earth from galaxies billions of light years away.
In April 2020, one of the bursts was for the first time detected from within our galaxy, the Milky Way, by radio telescopes CHIME and STARE2. The unexpected flare was traced to a previously-known source only 25 000 light years from Earth in the constellation of Vulpecula, the Fox, and scientists all over the world coordinated their efforts to follow up the discovery.
In May, a team of scientists led by Franz Kirsten (Chalmers) pointed four of Europe’s best radio telescopes towards the source, known as SGR 1935+2154. Their results are published today in a paper in the journal Nature Astronomy.
“We didn’t know what to expect. Our radio telescopes had only rarely been able to see fast radio bursts, and this source seemed to be doing something completely new. We were hoping to be surprised!”, said Mark Snelders, team member from the Anton Pannekoek Institute for Astronomy, University of Amsterdam.
The radio telescopes, one dish in Westerbork (Netherlands), one dish in Poland and two at Onsala Space Observatory in Sweden, monitored the source every night for more than four weeks after the discovery of the first flash, a total of 522 hours of observation.
On the evening of May 24, the team got the surprise they were looking for. At 23:19 local time, ASTRON's Westerbork Synthesis Radio Telescope (WSRT) in the Netherlands, the only one of the group on duty, caught a dramatic and unexpected signal: two short bursts, each one millisecond long but 1.4 seconds apart.
Kenzie Nimmo, astronomer at ASTRON and Anton Pannekoek Institute for Astronomy , is a member of the team.
“We clearly saw two bursts, extremely close in time. Like the flash seen from the same source on April 28, this looked just like the fast radio bursts we’d been seeing from the distant universe, only dimmer. The two bursts we detected on May 24 were even fainter than that”, she said.
This was new, strong evidence connecting fast radio bursts with magnetars, the scientists thought. Like more distant sources of fast radio bursts, SGR 1935+2154 seemed to be producing bursts at random intervals, and over a huge brightness range.
“The brightest flashes from this magnetar are at least ten million times as bright as the faintest ones. We asked ourselves, could that also be true for fast radio burst sources outside our galaxy? If so, then the universe’s magnetars are creating beams of radio waves that could be criss-crossing the cosmos all the time – and many of these could be within the reach of modest-sized telescopes like ours”, said team member Jason Hessels (ASTRON and Anton Pannekoek Institute for Astronomy).
Neutron stars are the tiny, extremely dense remnants left behind when a short-lived star of more than eight times the mass of the Sun explodes as a supernova. For 50 years, astronomers have studied pulsars, neutron stars which with clock-like regularity send out pulses of radio waves and other radiation. All pulsars are believed to have strong magnetic fields, but the magnetars are the strongest known magnets in the universe, each with a magnetic field hundreds of trillions of times stronger than the Sun’s.
In the future, the team aims to keep the radio telescopes monitoring SGR 1935+2154 and other nearby magnetars, in the hope of pinning down how these extreme stars actually make their brief blasts of radiation.
Scientists have presented many ideas for how fast radio bursts are generated. Franz Kirsten, astronomer at Onsala Space Observatory, Chalmers, who led the project, expects the rapid pace in understanding the physics behind fast radio bursts to continue.
“The fireworks from this amazing, nearby magnetar have given us exciting clues about how fast radio bursts might be generated. The bursts we detected on May 24 could indicate a dramatic disturbance in the star’s magnetosphere, close to its surface. Other possible explanations, like shock waves further out from the magnetar, seem less likely, but I’d be delighted to be proved wrong. Whatever the answers, we can expect new measurements and new surprises in the months and years to come”, he said.
More about the research and the telescopes
The research is published in a paper “Detection of two bright radio bursts from magnetar SGR 1935+2154” in Nature Astronomy, by Franz Kirsten (Onsala Space Observatory, Chalmers), M. P. Snelders, M. Jenkins (Anton Pannekoek Institute for Astronomy, University of Amsterdam) K. Nimmo (ASTRON, Netherlands Institute for Radio Astronomy, and Anton Pannekoek Institute for Astronomy, University of Amsterdam), J. van den Eijnden (Anton Pannekoek Institute for Astronomy, University of Amsterdam and Department of Physics, Astrophysics, University of Oxford), J. W. T. Hessels (ASTRON, Netherlands Institute for Radio Astronomy, and Anton Pannekoek Institute for Astronomy, University of Amsterdam), M. P. Gawroński (Institute of Astronomy, Nicolaus Copernicus University, Toruń, Poland) and Jun Yang (Onsala Space Observatory, Chalmers).
The observations were carried out using the 25-metre RT1 telescope at Westerbork, Netherlands, both the 25-metre and 20-metre telescopes at Onsala Space Observatory, and the 32-metre telescope in Toruń, Poland.