GECAM discovery of a peculiar magnetar X-ray burst (MXB 221120) from SGR J1935+2154 associated with a fast radio burst

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Tan, Wen-Jun, Wang, Yue, Wang, Chen-Wei, Xiong, Shao-Lin, Li, Xiao-Bo, Zhang, Shuang-Nan, Cai, Ce, Xue, Wang-Chen, Zhang, Peng, Wu, Bo-Bing, An, Zheng-Hua, Gao, Ming, Ge, Ming-Yu, Gong, Ke, Guo, Dong-Ya, Guo, Hao-Xuan, Hao, Long-Fei, Huang, Yue, Huang, Yu-Xiang, Lee, Ke-Jia, Li, Bing, Li, Kui-Cheng, Li, Xin-Qiao, Liu, Jia-Cong, Liu, Xiao-Jing, Liu, Ya-Qing, Ma, Xiang, Peng, Wen-Xi, Qiao, Rui, Ren, Yang-Zhao, Song, Li-Ming, Sun, Xi-Lei, Wang, Jin, Wang, Jin-Zhou, Wang, Ping, Wen, Xiang-Yang, Xiao, Shuo, Xie, Lun-Sheng, Xu, Heng, Yang, Sheng, Yi, Shu-Xu, Yi, Qi-bin, Yu, Zheng-Hang, Zhang, Li-Da, Zhang, Fan, Zhang, Hong-Mei, Zhang, Jin-Peng, Zhang, Yan-Qiu, Zhang, Zhen, Zhao, Xiao-Yun, Zhao, Yi, Zheng, Chao, Zheng, Shi-Jie
Format: Preprint
Veröffentlicht: 2026
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866908933761794048
author Tan, Wen-Jun
Wang, Yue
Wang, Chen-Wei
Xiong, Shao-Lin
Li, Xiao-Bo
Zhang, Shuang-Nan
Cai, Ce
Xue, Wang-Chen
Zhang, Peng
Wu, Bo-Bing
An, Zheng-Hua
Gao, Ming
Ge, Ming-Yu
Gong, Ke
Guo, Dong-Ya
Guo, Hao-Xuan
Hao, Long-Fei
Huang, Yue
Huang, Yu-Xiang
Lee, Ke-Jia
Li, Bing
Li, Kui-Cheng
Li, Xin-Qiao
Liu, Jia-Cong
Liu, Xiao-Jing
Liu, Ya-Qing
Ma, Xiang
Peng, Wen-Xi
Qiao, Rui
Ren, Yang-Zhao
Song, Li-Ming
Sun, Xi-Lei
Wang, Jin
Wang, Jin-Zhou
Wang, Ping
Wen, Xiang-Yang
Xiao, Shuo
Xie, Lun-Sheng
Xu, Heng
Yang, Sheng
Yi, Shu-Xu
Yi, Qi-bin
Yu, Zheng-Hang
Zhang, Li-Da
Zhang, Fan
Zhang, Hong-Mei
Zhang, Jin-Peng
Zhang, Yan-Qiu
Zhang, Zhen
Zhao, Xiao-Yun
Zhao, Yi
Zheng, Chao
Zheng, Shi-Jie
author_facet Tan, Wen-Jun
Wang, Yue
Wang, Chen-Wei
Xiong, Shao-Lin
Li, Xiao-Bo
Zhang, Shuang-Nan
Cai, Ce
Xue, Wang-Chen
Zhang, Peng
Wu, Bo-Bing
An, Zheng-Hua
Gao, Ming
Ge, Ming-Yu
Gong, Ke
Guo, Dong-Ya
Guo, Hao-Xuan
Hao, Long-Fei
Huang, Yue
Huang, Yu-Xiang
Lee, Ke-Jia
Li, Bing
Li, Kui-Cheng
Li, Xin-Qiao
Liu, Jia-Cong
Liu, Xiao-Jing
Liu, Ya-Qing
Ma, Xiang
Peng, Wen-Xi
Qiao, Rui
Ren, Yang-Zhao
Song, Li-Ming
Sun, Xi-Lei
Wang, Jin
Wang, Jin-Zhou
Wang, Ping
Wen, Xiang-Yang
Xiao, Shuo
Xie, Lun-Sheng
Xu, Heng
Yang, Sheng
Yi, Shu-Xu
Yi, Qi-bin
Yu, Zheng-Hang
Zhang, Li-Da
Zhang, Fan
Zhang, Hong-Mei
Zhang, Jin-Peng
Zhang, Yan-Qiu
Zhang, Zhen
Zhao, Xiao-Yun
Zhao, Yi
Zheng, Chao
Zheng, Shi-Jie
contents Fast radio bursts (FRBs) are enigmatic cosmic transients of millisecond duration observed in the radio band. The identification of FRB-associated magnetar X-ray bursts (MXBs) from galactic magnetar SGR J1935+2154 suggests that at least a fraction of FRBs can be produced from magnetar activity. However, the sample size of FRB-associated MXBs is still very small. Here we report a bright and peculiar FRB-associated MXB from SGR J1935+2154 detected by GECAM on November 20, 2022, dubbed MXB 221120. We find that both temporal and spectral properties of MXB 221120 exhibit distinctive features. Its light curve could be generally described by a single FRED function with superposition of several narrow pulses. Interestingly, we identify a possible QPO feature with center frequency of ~18 Hz in this MXB. The time-integrated spectrum is best fitted by a blackbody model with temperature (kT ) of 18.6 keV, rendering it the first thermal spectrum FRB-associated MXB from SGR J1935+2154. Compared to other MXBs with single emission episode, MXB 221120 has longer duration and higher blackbody temperature, making it an outlier in the burst sample. These results indicate that MXB 221120 may be produced by a special mechanism with extreme physical conditions.
format Preprint
id arxiv_https___arxiv_org_abs_2604_02261
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle GECAM discovery of a peculiar magnetar X-ray burst (MXB 221120) from SGR J1935+2154 associated with a fast radio burst
Tan, Wen-Jun
Wang, Yue
Wang, Chen-Wei
Xiong, Shao-Lin
Li, Xiao-Bo
Zhang, Shuang-Nan
Cai, Ce
Xue, Wang-Chen
Zhang, Peng
Wu, Bo-Bing
An, Zheng-Hua
Gao, Ming
Ge, Ming-Yu
Gong, Ke
Guo, Dong-Ya
Guo, Hao-Xuan
Hao, Long-Fei
Huang, Yue
Huang, Yu-Xiang
Lee, Ke-Jia
Li, Bing
Li, Kui-Cheng
Li, Xin-Qiao
Liu, Jia-Cong
Liu, Xiao-Jing
Liu, Ya-Qing
Ma, Xiang
Peng, Wen-Xi
Qiao, Rui
Ren, Yang-Zhao
Song, Li-Ming
Sun, Xi-Lei
Wang, Jin
Wang, Jin-Zhou
Wang, Ping
Wen, Xiang-Yang
Xiao, Shuo
Xie, Lun-Sheng
Xu, Heng
Yang, Sheng
Yi, Shu-Xu
Yi, Qi-bin
Yu, Zheng-Hang
Zhang, Li-Da
Zhang, Fan
Zhang, Hong-Mei
Zhang, Jin-Peng
Zhang, Yan-Qiu
Zhang, Zhen
Zhao, Xiao-Yun
Zhao, Yi
Zheng, Chao
Zheng, Shi-Jie
High Energy Astrophysical Phenomena
Fast radio bursts (FRBs) are enigmatic cosmic transients of millisecond duration observed in the radio band. The identification of FRB-associated magnetar X-ray bursts (MXBs) from galactic magnetar SGR J1935+2154 suggests that at least a fraction of FRBs can be produced from magnetar activity. However, the sample size of FRB-associated MXBs is still very small. Here we report a bright and peculiar FRB-associated MXB from SGR J1935+2154 detected by GECAM on November 20, 2022, dubbed MXB 221120. We find that both temporal and spectral properties of MXB 221120 exhibit distinctive features. Its light curve could be generally described by a single FRED function with superposition of several narrow pulses. Interestingly, we identify a possible QPO feature with center frequency of ~18 Hz in this MXB. The time-integrated spectrum is best fitted by a blackbody model with temperature (kT ) of 18.6 keV, rendering it the first thermal spectrum FRB-associated MXB from SGR J1935+2154. Compared to other MXBs with single emission episode, MXB 221120 has longer duration and higher blackbody temperature, making it an outlier in the burst sample. These results indicate that MXB 221120 may be produced by a special mechanism with extreme physical conditions.
title GECAM discovery of a peculiar magnetar X-ray burst (MXB 221120) from SGR J1935+2154 associated with a fast radio burst
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2604.02261