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The Observer's Guide to the Gamma-Ray Burst Supernova Connection
Cano, Zach1,2; Wang, Shan-Qin3,4; Dai, Zi-Gao3,4; Wu, Xue-Feng5,6
2017
Source PublicationADVANCES IN ASTRONOMY
ISSN1687-7969
Pages41
Corresponding AuthorCano, Zach(zewcano@gmail.com)
AbstractWe 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.
DOI10.1155/2017/8929054
WOS KeywordCORE-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
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000399077100001
PublisherHINDAWI LTD
Citation statistics
Cited Times:58[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/23127
Collection中国科学院紫金山天文台
Corresponding AuthorCano, Zach
Affiliation1.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
Recommended Citation
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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