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Magnetar Flare-driven Bumpy Declining Light Curves in Hydrogen-poor Superluminous Supernovae

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成果类型:
期刊论文
作者:
Dong, Xiao-Fei;Liu, Liang-Duan;Gao, He;Yang, Sheng
通讯作者:
Liu, LD
作者机构:
[Gao, He; Dong, Xiao-Fei] Beijing Normal Univ, Inst Frontier Astron & Astrophys, Beijing 100875, Peoples R China.
[Gao, He; Dong, Xiao-Fei] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China.
[Liu, Liang-Duan; Liu, LD] Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China.
[Liu, Liang-Duan; Liu, LD] Cent China Normal Univ, Key Lab Quark & Lepton Phys, Minist Educ, Wuhan 430079, Peoples R China.
[Yang, Sheng] Henan Acad Sci, Zhengzhou 450046, Henan, Peoples R China.
通讯机构:
[Liu, LD ] C
Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Peoples R China.
Cent China Normal Univ, Key Lab Quark & Lepton Phys, Minist Educ, Wuhan 430079, Peoples R China.
语种:
英文
期刊:
ASTROPHYSICAL JOURNAL
ISSN:
0004-637X
年:
2023
卷:
951
期:
1
基金类别:
We thank Zongkai Peng, Zhihao Chen, and Shaoze Li for helpful comments and discussions, and the anonymous referee for important suggestions. This work is supported by the National Natural Science Foundation of China (Projects 12021003), the National SKA Program of China (2022SKA0130100), and the National Key R&D Program of China (2021YFA0718500). The ZTF forced-photometry service was funded under the Heising-Simons Foundation grant No. 12540303 (PI: Graham).
机构署名:
本校为通讯机构
院系归属:
物理科学与技术学院
摘要:
Recent observations indicate that hydrogen-poor superluminous supernovae (SLSNe-I) often display bumpy declining light curves. However, the cause of these undulations remains unclear. In this paper, we have improved the magnetar model, which includes flare activities. We present a systematic analysis of a well-observed SLSN-I sample with bumpy light curves in their late phase. These SLSNe-I were identified from multiple transient surveys, such as the Pan-STARRS1 Medium Deep Survey and the Zwicky Transient Facility. Our study provides a set of m...

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