中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
HXMT identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428

文献类型:期刊论文

作者Li, C. K.; Lin, L.; Xiong, S. L.; Ge, M. Y.; Li, X. B.; Li, T. P.; Lu, F. J.; Zhang, S. N.; Tuo, Y. L.; Nang, Y.
刊名Nature Astronomy
出版日期2021
ISSN号2397-3366
DOI10.1038/s41550-021-01302-6
英文摘要Fast radio bursts (FRBs) are short pulses observed in the radio band from cosmological distances1. One class of models invokes soft gamma-ray repeaters (SGRs), or magnetars, as the sources of FRBs2. Some radio pulses have been observed from some magnetars3, but no FRB-like events have been detected in association with any magnetar burst, including one giant flare4. Recently, a pair of FRB-like bursts (termed FRB 200428) separated by 29 milliseconds were detected from the general direction of the Galactic magnetar SGR J1935+2154 (refs. 5,6). Here, we report the detection of a non-thermal X-ray burst in the 1-250 keV energy band with the Insight-HXMT satellite7, which we identify as having been emitted from SGR J1935+2154. The burst showed two hard peaks with a separation of 34 milliseconds, broadly consistent with that of the two bursts in FRB 200428. The delay time between the double radio peak and the X-ray peaks is about 8.62 s, fully consistent with the dispersion delay of FRB 200428. We thus identify the non-thermal X-ray burst to be associated with FRB 200428, whose high-energy counterpart is the two hard X-ray peaks. Our results suggest that the non-thermal X-ray burst and FRB 200428 share the same physical origin in an explosive event from SGR J1935+2154.
WOS记录号WOS:000619391500003
源URL[http://ir.ihep.ac.cn/handle/311005/289777]  
专题高能物理研究所_粒子天体物理中心
硬X射线调制望远镜卫星
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Li, C. K.,Lin, L.,Xiong, S. L.,et al. HXMT identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428[J]. Nature Astronomy,2021.
APA Li, C. K..,Lin, L..,Xiong, S. L..,Ge, M. Y..,Li, X. B..,...&Zhuang, R. L..(2021).HXMT identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428.Nature Astronomy.
MLA Li, C. K.,et al."HXMT identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428".Nature Astronomy (2021).

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来源:高能物理研究所

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