Origins of Fast Radio Bursts
- 26 May 2023
Recently, a study by a team of astronomers uncovered significant insights into fast radio bursts (FRBs).
About FRBs: FRBs are fleeting bursts of radio waves from distant galaxies that have puzzled scientists for over 15 years.
About the Study: The study focused on a repeating FRB, FRB 20190520B, allowing researchers to investigate its local environment and shed light on its sources.
Key Findings
- Highly Variable Faraday Rotation Measure: The FRB’s Faraday rotation measure – an indicator of its magnetic field strength – was highly variable.
- Researchers observed two instances of magnetic field reversal, suggesting that the FRB source orbits a binary star system with a massive star or black hole companion.
- Variations in Magnetic Field Strength: The observations also revealed variations in magnetic field strength and electron density around the FRB source, indicating a turbulent and magnetized plasma environment.
- Wind Emitted by a Massive Companion Star: Models constructed by the scientists attribute these variations to a wind emitted by a massive companion star in the binary system.
- FRB Originated from a Binary System: This study provides compelling evidence that this FRB originated from a binary system, and it suggests that all repeating FRBs may be associated with binaries, albeit with different local conditions.
- Understanding changes in the magnetized environment around FRBs is crucial for revealing their origins.
Pulsars are rotating neutron stars observed to have pulses of radiation at very regular intervals that typically range from milliseconds to seconds. |