Insights into the X-Ray Burst Pulse Morphology from SGR J1935+2154

• Published in: The Astrophysical journal. Supplement series Vol. 279; no. 1; pp. 14 - 26
• Main Authors: Yang, Jiao-Jiao, Xiao, Shuo, Wang, Yue, Xiong, Shao-Lin, Lin, Lin, Jiang, Zheng-Huo, Liao, Tong-Lei, Li, Xiao-Bo, Li, Cheng-Kui, Yi, Shu-Xu, Zhang, Zhen, Zhang, Shuang-Nan
• Format: Journal Article
• Language: English
• Published: Saskatoon The American Astronomical Society 01.07.2025; IOP Publishing
• Subjects: Correlation; Decay; Gamma ray bursts; Gamma rays; Gravitational waves; Magnetars; Milky Way; Normal distribution; Parameters; Pulse duration; Radio bursts; X ray telescopes; X-ray bursts; X-rays

SGR J1935+2154 is an extremely active magnetar and the source of the first fast radio burst in the Milky Way, characterized as a magnetar X-ray burst, but whether the temporal features of this magnetar are specific or not is not well known. Based on data from the Fermi Gamma-ray Burst Monitor (GBM),...