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A peculiar low-luminosity short gamma-ray burst from a double neutron star merger progenitor
Zhang, B. -B.1,2,3; Zhang, B.4,5,6; Sun, H.7; Lei, W. -H.8; Gao, H.9; Li, Y.6; Shao, L.10,11; Zhao, Y.12; Hu, Y. -D.2,13; Lu, H. -J.14; Wu, X. -F.11,15; Fan, X. -L.16; Wang, G.17,18; Castro-Tirado, A. J.2,19; Zhang, S.10; Yu, B. -Y.10; Cao, Y. -Y.10; Liang, E. -W.14
2018-01-31
Source PublicationNATURE COMMUNICATIONS
ISSN2041-1723
Volume9Pages:6
Corresponding AuthorZhang, B. -B.(zhang.grb@gmail.com) ; Zhang, B.(zhang@physics.unlv.edu)
AbstractDouble neutron star (DNS) merger events are promising candidates of short gamma-ray burst (sGRB) progenitors as well as high-frequency gravitational wave (GW) emitters. On August 17, 2017, such a coinciding event was detected by both the LIGO-Virgo gravitational wave detector network as GW170817 and Gamma-Ray Monitor on board NASA's Fermi Space Telescope as GRB 170817A. Here, we show that the fluence and spectral peak energy of this sGRB fall into the lower portion of the distributions of known sGRBs. Its peak isotropic luminosity is abnormally low. The estimated event rate density above this luminosity is at least 190(-160)(+440) Gpc(-3) yr(-1), which is close to but still below the DNS merger event rate density. This event likely originates from a structured jet viewed from a large viewing angle. There are similar faint soft GRBs in the Fermi archival data, a small fraction of which might belong to this new population of nearby, low-luminosity sGRBs.
DOI10.1038/s41467-018-02847-3
WOS KeywordGRAVITATIONAL-WAVE EVENT ; ELECTROMAGNETIC COUNTERPARTS ; GW170817 ; CATALOG ; GRBS
Indexed BySCI
Language英语
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
WOS IDWOS:000423674100003
PublisherNATURE PUBLISHING GROUP
Citation statistics
Cited Times:49[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/22221
Collection中国科学院紫金山天文台
Corresponding AuthorZhang, B. -B.; Zhang, B.
Affiliation1.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
2.Inst Astrofis Andalucia IAA CSIC, POB 03004, E-18080 Granada, Spain
3.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210093, Peoples R China
4.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
5.Peking Univ, Dept Astron, Sch Phys, Beijing 100871, Peoples R China
6.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
7.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China
8.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Hubei, Peoples R China
9.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
10.Hebei Normal Univ, Dept Space Sci & Astron, Shijiazhuang 050024, Hebei, Peoples R China
11.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
12.Univ Florida, Dept Astron, Bryant Space Sci Ctr 211, Gainesville, FL 32611 USA
13.Univ Granada, Fac Ciencias, Campus Fuentenueva S-N, E-18071 Granada, Spain
14.Guangxi Univ, Guangxi Key Lab Relativist Astrophys, Dept Phys, Nanning 530004, Peoples R China
15.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China
16.Hubei Univ Educ, Sch Phys & Elect Informat, Wuhan 430205, Hubei, Peoples R China
17.Gran Sasso Sci Inst INFN, Via Francesco Crispi 7, I-67100 Laquila, Italy
18.INFN, Sez Pisa, Edificio C,Largo Bruno Pontecorvo,3, I-56127 Pisa, Italy
19.Univ Malaga, Dept Ingn Sistemas & Automat, Escuela Ingn, C Dr Ortiz Ramos Sn, E-29071 Malaga, Spain
Recommended Citation
GB/T 7714
Zhang, B. -B.,Zhang, B.,Sun, H.,et al. A peculiar low-luminosity short gamma-ray burst from a double neutron star merger progenitor[J]. NATURE COMMUNICATIONS,2018,9:6.
APA Zhang, B. -B..,Zhang, B..,Sun, H..,Lei, W. -H..,Gao, H..,...&Liang, E. -W..(2018).A peculiar low-luminosity short gamma-ray burst from a double neutron star merger progenitor.NATURE COMMUNICATIONS,9,6.
MLA Zhang, B. -B.,et al."A peculiar low-luminosity short gamma-ray burst from a double neutron star merger progenitor".NATURE COMMUNICATIONS 9(2018):6.
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