X-Ray Hardening Preceding the Onset of SGR 1935+2154's Radio Pulsar Phase

X-Ray Hardening Preceding the Onset of SGR 1935+2154's Radio Pulsar Phase

Magnetars are neutron stars with extremely strong magnetic fields, frequently powering high-energy activity in X-rays. Pulsed radio emission following some X-ray outbursts has been detected, albeit its physical origin is unclear. It has long been speculated that the origin of magnetars’ radio signal...

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Main Authors: Pei Wang, Jian Li, Long Ji, Xian Hou, Erbil Gügercinoğlu, Di Li, Diego F. Torres, Yutong Chen, Jiarui Niu, Wei-Wei Zhu, Bing Zhang, En-Wei Liang, Li Zhang, Mingyu Ge, Zigao Dai, Lin Lin, Jinlin Han, Yi Feng, Chenhui Niu, Yongkun Zhang, Dejiang Zhou, Heng Xu, Chunfeng Zhang, Jinchen Jiang, Chenchen Miao, Mao Yuan, Weiyang Wang, Dengke Zhou, Jianhua Fang, Youling Yue, Yunsheng Wu, Yabiao Wang, Chengjie Wang, Zhenye Gan, Yuxi Li, Zhongyi Sun, Mingmin Chi, Junshuo Zhang, Jinhuang Cao, Wanjin Lu, Yidan Wang
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Magnetars
Online Access:https://doi.org/10.3847/1538-4365/ad7c3f
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https://doi.org/10.3847/1538-4365/ad7c3f

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