Signature of a Magnetar Central Engine from the Multiband Afterglow of GRB 151027A Associated with a Supernova

Abstract We report multiwavelength observations and theoretical modeling of the afterglow of gamma-ray burst (GRB) 151027A. The object exhibits a complete evolutionary sequence, including prompt gamma-ray and optical emission, an initial optical onset bump, an optical rebrightening, a late-time supernova bump, an X-ray flare, and two distinct X-ray plateaus. GRB 151027A exhibits nearly all characteristic features observed in GRB afterglows. Such a rich set of features within a single event is exceptionally rare. We show that the first X-ray plateau followed by a rapid decay can be attributed to the collapse of a newly formed magnetar to form a black hole. The second X-ray plateau can be explained by fallback accretion. We find that the energy-injection model successfully reproduces the optical rebrightening of GRB 151027A. The late-time optical bump is well described by a 56 Ni-powered supernova light curve. GRB 151027A presents a complete physical picture for GRB phenomenology, whereas reconstructing such a comprehensive picture previously required the statistical analysis of multiple GRBs.

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Publication Details

Journal
The Astrophysical Journal
Published
2026-04-28
DOI
https://doi.org/10.3847/1538-4357/ae595e
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
0.00

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article

Signature of a Magnetar Central Engine from the Multiband Afterglow of GRB 151027A Associated with a Supernova

Hou-Jun Lü, B Zhang, Y. D. Hu, D. A. Perley et al.
The Astrophysical Journal
Gamma-ray bursts and supernovae
article

Signature of a Magnetar Central Engine from the Multiband Afterglow of GRB 151027A Associated with a Supernova

Hou-Jun Lü, B Zhang, Y. D. Hu, D. A. Perley, Liang-Jun Chen, De-Feng Kong, S. Bradley Cenko, Hong-Bang Liu, Da-Bin Lin, Yihan Wang, Xiang-Gao Wang, WeiKang Zheng, Alexei V. Filippenko, Jie Xia, Fei Xie, Jing Lü, En-Wei Liang
article en

Abstract

Abstract We report multiwavelength observations and theoretical modeling of the afterglow of gamma-ray burst (GRB) 151027A. The object exhibits a complete evolutionary sequence, including prompt gamma-ray and optical emission, an initial optical onset bump, an optical rebrightening, a late-time supernova bump, an X-ray flare, and two distinct X-ray plateaus. GRB 151027A exhibits nearly all characteristic features observed in GRB afterglows. Such a rich set of features within a single event is exceptionally rare. We show that the first X-ray plateau followed by a rapid decay can be attributed to the collapse of a newly formed magnetar to form a black hole. The second X-ray plateau can be explained by fallback accretion. We find that the energy-injection model successfully reproduces the optical rebrightening of GRB 151027A. The late-time optical bump is well described by a 56 Ni-powered supernova light curve. GRB 151027A presents a complete physical picture for GRB phenomenology, whereas reconstructing such a comprehensive picture previously required the statistical analysis of multiple GRBs.

The Astrophysical JournalVol. 1002(1)
University of Science and Technology of China (CN), Goddard Space Flight Center (US), University of Nevada, Las Vegas (US), University of Wisconsin–Madison (US), Guangxi University (CN), Purple Mountain Observatory (CN), Deleted Institution, Liverpool John Moores University (GB), University of Hong Kong (HK), University of California, Berkeley (US)
National Natural Science Foundation of China
Openalex Percentile: Top 9%
Gamma-ray bursts and supernovae
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