Polarization Position Angle Swing and the Rotating Vector Model of Repeating Fast Radio Bursts

Polarization Position Angle Swing and the Rotating Vector Model of Repeating Fast Radio Bursts

Fast radio bursts (FRBs), typically highly polarized, usually have a nearly constant polarization position angle (PA) during each burst. Some bursts show significant PA variations, and one of them was claimed to have a PA variation pattern consistent with the prediction of the rotating vector model...

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Bibliographic Details
Main Authors: Xiaohui Liu, Heng Xu, Jiarui Niu, Yongkun Zhang, Jinchen Jiang, Dejiang Zhou, Jinlin Han, Weiwei Zhu, Kejia Lee, Di Li, Wei-Yang Wang, Bing Zhang, Xuelei Chen, Jia-Wei Luo, Rui Luo, Chenhui Niu, Yuanhong Qu, Bojun Wang, Fayin Wang, Pei Wang, Tiancong Wang, Qin Wu, Ziwei Wu, Jiangwei Xu, Yuan-Pei Yang, Jun-Shuo Zhang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Radio bursts
Neutron stars
Radio transient sources
Online Access:https://doi.org/10.3847/1538-4357/ade689
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https://doi.org/10.3847/1538-4357/ade689

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