A sudden change and recovery in the magnetic environment around a repeating fast radio burst

Fast radio bursts (FRBs) are millisecond-duration radio transients from extragalactic sources. Some repeating FRBs exhibit variations in their Faraday rotation measure (RM) due to changes in their magneto-ionic environment. We report magneto-ionic variations of FRB 20220529, a repeating FRB from a disk galaxy at redshift 0.18. For the first 17 months of observations, the RM had a median of 17 radians per square meter (rad m<sup>-2</sup>) and a scatter of 101 rad m<sup>-2</sup>. In December 2023, the RM jumped to 1977 ± 84 rad m<sup>-2</sup>, then gradually returned to typical values within 2 weeks. This sudden RM variation indicates that a dense magnetized clump of plasma passed across the line of sight. We discuss potential explanations, including a coronal mass ejection from a companion star, high plasma turbulence, or binary orbital motion.

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Publication Details

Journal
Science
Published
2026-01-15
DOI
https://doi.org/10.1126/science.adq3225
Citations
2
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
47.65
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article

A sudden change and recovery in the magnetic environment around a repeating fast radio burst

Chong Niu, Jin-Jun Geng, X. L. Chen, Kaitlyn Shin et al.
2 citations
Science
Pulsars and Gravitational Waves Research
47.65
article

A sudden change and recovery in the magnetic environment around a repeating fast radio burst

Chong Niu, Jin-Jun Geng, X. L. Chen, Kaitlyn Shin, Peng Jiang, Zhifeng Tang, C. J. Law, T. R. Sun, B. J. Wang, Y. K. Zhang, Rui Luo, J. R. Niu, Dongzi Li, Songbo Zhang, C. F. Zhang, Ryan Mckinven, Dong Shi, Zi-Gao Dai, Yibin Feng, Xue-Feng Wu, Di Li, Xuan Yang, George Chen, Yan Zhu, Chen‐Ming Chang, B. Zhang, C. W. Tsai, Xiaoli Yang, H. Xu, L. Hu, R. Anna-Thomas, Y. Li, D. Xiao, D. J. Zhou, J. L. Han, Y. P. Yang, K. J. Lee, W. W. Zhu
article en
2 citations

Abstract

Fast radio bursts (FRBs) are millisecond-duration radio transients from extragalactic sources. Some repeating FRBs exhibit variations in their Faraday rotation measure (RM) due to changes in their magneto-ionic environment. We report magneto-ionic variations of FRB 20220529, a repeating FRB from a disk galaxy at redshift 0.18. For the first 17 months of observations, the RM had a median of 17 radians per square meter (rad m<sup>-2</sup>) and a scatter of 101 rad m<sup>-2</sup>. In December 2023, the RM jumped to 1977 ± 84 rad m<sup>-2</sup>, then gradually returned to typical values within 2 weeks. This sudden RM variation indicates that a dense magnetized clump of plasma passed across the line of sight. We discuss potential explanations, including a coronal mass ejection from a companion star, high plasma turbulence, or binary orbital motion.

ScienceVol. 391(6782)
West Virginia University (US), California Institute of Technology (US), University of Science and Technology of China (CN), Australia Telescope National Facility (AU), University of Nevada, Las Vegas (US), Guizhou University (CN), Anhui University of Science and Technology (CN), Yunnan University (CN), Chinese Academy of Sciences (CN), Princeton University (US), Peking University (CN), Beijing Normal University (CN), Shanghai Astronomical Observatory (CN), Purple Mountain Observatory (CN), Guangzhou University (CN), National Time Service Center (CN), Kavli Institute for Theoretical Sciences (CN), Zhejiang Lab (CN), Astronomy and Space (AU), National Astronomical Observatories (CN), McGill University (CA), Massachusetts Institute of Technology (US), Carnegie Mellon University (US), Zhejiang University (CN), University of Pennsylvania (US), University of Amsterdam (NL), University of Hong Kong (HK), Netherlands Institute for Radio Astronomy (NL), Tsinghua University (CN)
Openalex Percentile: Top 1%
Pulsars and Gravitational Waves Research
47.65
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