The Observer's Guide to the Gamma-Ray Burst Supernova Connection
文献类型：期刊论文
| 作者 | Cano, Zach1,2; Wang, Shan-Qin3,4; Dai, Zi-Gao3,4; Wu, Xue-Feng5,6
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| 刊名 | ADVANCES IN ASTRONOMY
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| 出版日期 | 2017 |
| 页码 | 41 |
| ISSN号 | 1687-7969 |
| DOI | 10.1155/2017/8929054 |
| 通讯作者 | Cano, Zach(zewcano@gmail.com) |
| 英文摘要 | We present a detailed report of the connection between long-duration gamma-ray bursts (GRBs) and their accompanying supernovae (SNe). The discussion presented here places emphasis on how observations, and the modelling of observations, have constrained what we know about GRB-SNe. We discuss their photometric and spectroscopic properties, their role as cosmological probes, including their measured luminosity-decline relationships, and how they can be used to measure the Hubble constant. We present a statistical summary of their bolometric properties and use this to determine the properties of the "average" GRB-SN. We discuss their geometry and consider the various physical processes that are thought to power the luminosity of GRB-SNe and whether differences exist between GRB-SNe and the SNe associated with ultra-long-duration GRBs. We discuss how observations of their environments further constrain the physical properties of their progenitor stars and give a brief overview of the current theoretical paradigms of their central engines. We then present an overview of the radioactively powered transients that have been photometrically associated with short-duration GRBs, and we conclude by discussing what additional research is needed to further our understanding of GRB-SNe, in particular the role of binary-formation channels and the connection of GRB-SNe with superluminous SNe. |
| WOS关键词 | CORE-COLLAPSE SUPERNOVAE ; SPACE-TELESCOPE OBSERVATIONS ; STAR-FORMING GALAXIES ; BLACK-HOLE BINARIES ; 25 APRIL 1998 ; CONTINUOUS ENERGY INJECTION ; MASS-METALLICITY RELATION ; XMM-NEWTON OBSERVATIONS ; GRB OPTICAL AFTERGLOWS ; TRIPLE-RING NEBULA |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000399077100001 |
| 出版者 | HINDAWI LTD |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/23126]  |
| 专题 | 中国科学院紫金山天文台 |
| 通讯作者 | Cano, Zach |
| 作者单位 | 1.Univ Iceland, Ctr Astrophys & Cosmol, Sci Inst, Dunhagi 5, IS-107 Reykjavik, Iceland 2.CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, Granada 18008, Spain 3.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China 4.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing, Jiangsu, Peoples R China 5.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 6.Nanjing Univ, Joint Ctr Particle Nucl Phys & Cosmol, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China |
| 推荐引用方式 GB/T 7714 | Cano, Zach,Wang, Shan-Qin,Dai, Zi-Gao,et al. The Observer's Guide to the Gamma-Ray Burst Supernova Connection[J]. ADVANCES IN ASTRONOMY,2017:41. |
| APA | Cano, Zach,Wang, Shan-Qin,Dai, Zi-Gao,&Wu, Xue-Feng.(2017).The Observer's Guide to the Gamma-Ray Burst Supernova Connection.ADVANCES IN ASTRONOMY,41. |
| MLA | Cano, Zach,et al."The Observer's Guide to the Gamma-Ray Burst Supernova Connection".ADVANCES IN ASTRONOMY (2017):41. |
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来源：紫金山天文台
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