A 50 s Quasiperiodic Oscillation in the Early X-Ray Afterglow of GRB 220711B

It is generally believed that long-duration gamma-ray bursts (GRBs) originate from the core collapse of rapidly spinning massive stars, and at least some of them are powered by hyperaccreting black holes (BHs). However, definite proofs about the progenitor and central engine of these GRBs have not b...

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Bibliographic Details
Main Authors:	H. Gao, W.-H. Lei, S. Xiao, Z.-P. Zhu, L. Lan, S.-K. Ai, A. Li, N. Xu, T.-C. Wang, B. Zhang, D. Xu, J. P. U. Fynbo, K. E. Heintz, P. Jakobsson, D. A. Kann, S.-Y. Fu, S.-Q. Jiang, X. Liu, S.-L. Xiong, W.-X. Peng, X.-B. Li, W.-C. Xue
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/adc4e2
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A 50 s Quasiperiodic Oscillation in the Early X-Ray Afterglow of GRB 220711B

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