Study Pinpoints FRB 20221022A’s Origins
According to a study revealed in Nature, the staff from the Massachusetts Institute of Technology (MIT) examined FRB 20221022A, a burst detected from a galaxy 200 million light-years away. By analysing its scintillation — a phenomenon inflicting gentle to seem to twinkle — the researchers recognized the origin as being inside 10,000 kilometres of a neutron star, an space referred to as the magnetosphere. This marks the primary conclusive proof of FRBs rising from such a area.
Insights from Scintillation Analysis
As reported by Phys.org, the research revealed that the burst exhibited steep variations in brightness, indicative of scintillation attributable to fuel inside its host galaxy. This fuel served as a lens, permitting researchers to find out the burst’s proximity to its supply. Lead creator Dr. Kenzie Nimmo from MIT advised the publication the importance of finding the origin inside a whole bunch of hundreds of kilometres from the supply, contrasting it with theories suggesting farther shockwave origins.
Polarisation Patterns Suggest Rotation
Collaborators from McGill University discovered the burst’s gentle to be extremely polarised, forming an S-shaped curve—a function attribute of rotating neutron stars, also referred to as pulsars. This discovering additional helps the conclusion that FRBs originate from extremely magnetised environments.
Potential for Future Research
The research, involving consultants like Dr. Kiyoshi Masui and others, highlights the potential of scintillation as a software for pinpointing FRB origins. These findings pave the way in which for understanding the varied physics behind these enigmatic bursts, that are detected every day by superior telescopes like CHIME.
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