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astro-ph.HE2024
A new subclass of gamma-ray burst originating from compact binary merger
Chen-Wei Wang, Wen-Jun Tan, Shao-Lin Xiong +15
Type I gamma-ray bursts (GRBs) are believed to originate from compact binary merger usually with duration less than 2 seconds for the main emission. However, recent observations of…
astro-ph.HE2024★ 13 cited
Finding the Particularity of the Active Episode of SGR J1935+2154 during Which FRB 20200428 Occurred: Implication from Statistics of Fermi/GBM X-Ray Bursts
Sheng-Lun Xie, Yun-Wei Yu, Shao-Lin Xiong +5
By using the Fermi/Gamma-ray Burst Monitor data of the X-ray bursts (XRBs) of SGR J1935+2154, we investigate the temporal clustering of the bursts and the cumulative distribution o…