A team of astronomers has come closer to explaining the mysterious radio pulses from the outer space.
Astronomers have tied the origin of a Fast Radio Burst to a highly magnetized, gas-filled region of space, providing a new hint in the decade-long quest to explain the mysterious radio pulses.
“We now know that the energy from this particular burst passed through a dense magnetized field shortly after it formed,” says lead author Kiyoshi Masui of the University of British Columbia, adding that this significantly narrows down the source’s environment and type of event that triggered the burst and means the source of the pulse likely resides within a star-forming nebula or the remnant of a supernova.
Fast Radio Bursts (FRBs), bursts of energy from space that appear as a short flashes of radio waves to telescopes on Earth, have baffled astronomers since first detected a decade ago. While only 16 have ever been recorded, scientists believe there could be thousands of FRBs a day.
“Hidden within an incredibly massive dataset, we found a very peculiar signal that matched all the known characteristics of a Fast Radio Burst, but with a tantalizing extra element that we simply have never seen before,” said Jeffrey Peterson, one of the researchers.
In this case, the researchers found the FRB exhibited Faraday rotation, which is a corkscrew-like twist radio waves acquire by passing through a powerful magnetic field.
“Taken together, these remarkable data reveal more about an FRB than we have ever seen before and give us important constraints on these mysterious events,” said Masui.