Fast radio bursts, or FRBs, are bright, powerful emissions of radio waves ranging from a fraction of a millisecond to a few milliseconds, each producing energy equivalent to the sun’s annual output.
The emissions associated with FRB 20201124A occurred for 82 hours over 54 days in the spring of 2021, making it one of the most active known fast radio bursts. It was visible through the world’s largest radio telescope — the China-based Five-hundred-meter Aperture Spherical radio Telescope, or FAST.
During the first 36 days, the study team was surprised to see irregular, short-time variations of the Faraday rotation measure, which measures the strength of the magnetic field and density of particles in the surroundings of FRB 20201124A. A larger rotation measure means the magnetic field near the radio burst’s source is stronger, denser or both, and a smaller measure means the opposite, Bing Zhang, a coauthor of the study and astrophysicist, said via email.
“This is not reflective of the beginning of the FRB’s (life span),” said Zhang, the founding director of the Center for Astrophysics at the University of Nevada, Las Vegas. “The FRB source has been there for a long time but has been dormant most of the time. It occasionally wakes up (this time for 54 days) and emits a lot of bursts.”
The measures went up and down during that time period, then stopped during the last 18 days before the FRB dampened — “suggesting that the magnetic field strength and/or density along the line of sight in the vicinity of the FRB source are varying with time,” Zhang added. “It suggests that the environment of the FRB source is dynamically evolving, with rapidly changing magnetic fields or density or both.”
“I equate it to filming a movie of the surroundings of an FRB source, and our film revealed a complex, dynamically evolving, magnetized environment that was never imagined before,” Zhang said in a news release.
The radio burst’s complex, magnetized environment is within about an astronomical unit (the distance between Earth and the sun) from its source, the researchers found.
They also discovered that the burst originated from a barred spiral galaxy, which is metal-rich and similar in size to the Milky Way, by using the 10-meter Keck telescopes in Mauna Kea, Hawaii. The radio burst’s source is located between the galaxy’s spiral arms where no significant star formation is taking place, making it less likely the origin is solely a magnetar, according to Nature study coauthor Subo Dong, an associate professor at the Kavli Institute for Astronomy and Astrophysics at Peking University.
“Such an environment is not straightforwardly expected for an isolated magnetar,” Zhang said in a news release. “Something else might be in the vicinity of the FRB engine, possibly a binary companion.”
The modeling study should encourage further searches for fast radio burst signals from Be star/X-ray binaries, the authors said.
“These observations brought us back to the drawing board,” Zhang said. “It is clear that FRBs are more mysterious than what we have imagined. More multi-wavelength observational campaigns are needed to further unveil the nature of these objects.”