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The Observer's Guide to the Gamma-Ray Burst Supernova Connection
Cano, Zach; Wang, Shan-Qin; Dai, Zi-Gao; Wu, Xue-Feng
刊名ADVANCES IN ASTRONOMY
2017
页码8929054-
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.
语种英语
内容类型期刊论文
源URL[http://libir.pmo.ac.cn/handle/332002/17427]  
专题中国科学院紫金山天文台
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,2017:8929054-.
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,8929054-.
MLA Cano, Zach,et al."The Observer's Guide to the Gamma-Ray Burst Supernova Connection".ADVANCES IN ASTRONOMY (2017):8929054-.
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