GRB 111005A at z = 0.0133 and the Prospect of Establishing Long-Short GRB/GW Association
文献类型：期刊论文
| 作者 | Wang, Yuan-Zhu; Huang, Yong-Jia; Liang, Yun-Feng; Li, Xiang; Jin, Zhi-Ping; Zhang, Fu-Wen; Zou, Yuan-Chuan; Fan, Yi-Zhong; Wei, Da-Ming |
| 刊名 | The Astrophysical Journal
 |
| 出版日期 | 2017 |
| 卷号 | 851页码:L20 |
| 关键词 | gamma-ray burst: general gamma-ray burst: individual: GRB 111005A gravitational waves Astrophysics - High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology |
| ISSN号 | 0004-637X |
| DOI | 10.3847/2041-8213/aa9d7f |
| 文献子类 | Journal article (JA) |
| 英文摘要 | GRB 111005A, a long-duration gamma-ray burst (GRB) that occurred within a metal-rich environment that lacks massive stars with {M}{ZAMS}ݳlant 15 {M} , is not coincident with supernova emission down to a stringent limit and thus should be classified as a long-short GRB (lsGRB; also known as an SN-less long GRB or hybrid GRB), like GRB 060505 and GRB 060614. In this work, we show that in the neutron star merger model the non-detection of the optical/infrared emission of GRB 111005A requires sub-relativistic neutron-rich ejecta with a mass of ܳlant 0.01 {M} , which is (significantly) less massive than that of GRB 130603B, GRB 060614, GRB 050709, and GRB 170817A. The lsGRBs are found to have a high rate density and the neutron star merger origin model can be unambiguously tested by the joint observations of the second-generation gravitational- wave (GW) detectors and the full-sky gamma-ray monitors such as Fermi- GBM and the proposed GECAM. If no lsGRB/GW association is observed in the 2020s, alternative scenarios have to be systematically investigated. With the detailed environmental information achievable for the nearby events, a novel kind of merger or explosion origin may be identified. |
| 语种 | 英语 |
| WOS记录号 | WOS:000417542100020 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/287851]  |
| 专题 | 引力波暴高能电磁对应体全天监测器（GECAM） |
| 推荐引用方式 GB/T 7714 | Wang, Yuan-Zhu,Huang, Yong-Jia,Liang, Yun-Feng,et al. GRB 111005A at z = 0.0133 and the Prospect of Establishing Long-Short GRB/GW Association[J]. The Astrophysical Journal,2017,851:L20. |
| APA | Wang, Yuan-Zhu.,Huang, Yong-Jia.,Liang, Yun-Feng.,Li, Xiang.,Jin, Zhi-Ping.,...&Wei, Da-Ming.(2017).GRB 111005A at z = 0.0133 and the Prospect of Establishing Long-Short GRB/GW Association.The Astrophysical Journal,851,L20. |
| MLA | Wang, Yuan-Zhu,et al."GRB 111005A at z = 0.0133 and the Prospect of Establishing Long-Short GRB/GW Association".The Astrophysical Journal 851(2017):L20. |
入库方式： OAI收割
来源：高能物理研究所
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