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-Zhu1,2; Huang, Yong-Jia1,3; Liang, Yun-Feng1 ; Li, Xiang1; Jin, Zhi-Ping1,3; Zhang, Fu-Wen4; Zou, Yuan-Chuan5; Fan, Yi-Zhong1,3; Wei, Da-Ming1,3
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| 刊名 | ASTROPHYSICAL JOURNAL LETTERS
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| 出版日期 | 2017-12-10 |
| 卷号 | 851期号:1页码:5 |
| ISSN号 | 2041-8205 |
| 关键词 | gamma-ray burst: general gamma-ray burst: individual (GRB 111005A) gravitational waves |
| DOI | 10.3847/2041-8213/aa9d7f |
| 通讯作者 | Li, Xiang(xiangli@pmo.ac.cn) |
| 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 MZAMS >= 15M(circle dot), 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 <= 0.01 M-circle dot, 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. |
| WOS关键词 | GAMMA-RAY BURST ; R-PROCESS NUCLEOSYNTHESIS ; NEUTRON-STAR MERGER ; LUMINOSITY FUNCTION ; BINARY MERGERS ; CONNECTION ; GRB-060614 ; MACRONOVA ; SUPERNOVA ; SEARCH |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | IOP PUBLISHING LTD |
| WOS记录号 | WOS:000417542100020 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/22115]  |
| 专题 | 中国科学院紫金山天文台 |
| 通讯作者 | Li, Xiang |
| 作者单位 | 1.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 2.Univ Chinese Acad Sci, Yuquan Rd 19, Beijing 100049, Peoples R China 3.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China 4.Guilin Univ Technol, Coll Sci, Guilin 541004, Peoples R China 5.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Hubei, Peoples R China |
| 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]. ASTROPHYSICAL JOURNAL LETTERS,2017,851(1):5. |
| 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.ASTROPHYSICAL JOURNAL LETTERS,851(1),5. |
| MLA | Wang, Yuan-Zhu,et al."GRB 111005A at z=0.0133 and the Prospect of Establishing Long-Short GRB/GW Association".ASTROPHYSICAL JOURNAL LETTERS 851.1(2017):5. |
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来源：紫金山天文台
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