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Thermal and Nonthermal Emission from a Peculiar Long-duration GRB 211211A

Long-duration GRB 211211A that lacks a supernova emission even down to very stringent limits at such a low redshift z = 0.076 and is associated with kilonova emission, suggests that its physical origin is from a binary compact star merger. By reanalyzing its data observed with the Gamma-Ray Burst Mo...

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Bibliografski detalji
Glavni autori: Xue-Zhao Chang, Hou-Jun Lü, Xing Yang, Jia-Ming Chen, En-Wei Liang
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2023-01-01
Serija:The Astrophysical Journal
Teme:
Online pristup:https://doi.org/10.3847/1538-4357/aca969
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