A Subclass of Gamma-Ray Burst Originating from Compact Binary Merger

A Subclass of Gamma-Ray Burst Originating from Compact Binary Merger

Type I gamma-ray bursts (GRBs) are believed to originate from compact binary mergers usually with a duration of main emission less than 2 s. However, recent observations of GRB 211211A and GRB 230307A indicate that some merger-origin GRBs could last much longer. Since they show strikingly similar pr...

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Bibliographic Details
Main Authors: Chen-Wei Wang, Wen-Jun Tan, Shao-Lin Xiong, Shu-Xu Yi, Rahim Moradi, Bing Li, Zhen Zhang, Yu Wang, Yan-Zhi Meng, Bo-Bing Wu, Jia-Cong Liu, Yue Wang, Sheng-Lun Xie, Wang-Chen Xue, Zheng-Hang Yu, Peng Zhang, Wen-Long Zhang, Yan-Qiu Zhang, Chao Zheng
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Gamma-ray bursts
Online Access:https://doi.org/10.3847/1538-4357/ad98ec
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https://doi.org/10.3847/1538-4357/ad98ec

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