Spectroscopy of the Type Ic Supernova SN2017iuk Associated with Low-redshift GRB171205A

doi:10.3847/1538-4357/aae6c3

CORC > 国家天文台 > 中国科学院国家天文台

	Spectroscopy of the Type Ic Supernova SN2017iuk Associated with Low-redshift GRB171205A
	Wang, J.2,3; Zhu, Z. P.2,4; Xu, D.2; Xin, L. P.2; Deng, J. S.2,3; Qiu, Y. L.2; Qiu, P.1; Wang, H. J.1; Zhang, J. B.1; Wei, J. Y.2,3
刊名	ASTROPHYSICAL JOURNAL
	2018-11-10
卷号	867 期号:2 页码:7
关键词	gamma-ray burst: individual (GRB 171205A) methods: observational supernovae: individual (SN 2017iuk) techniques: spectroscopic
ISSN号	0004-637X
DOI	10.3847/1538-4357/aae6c3
英文摘要	We here report a spectroscopic monitor for the supernova (SN) SN 2017iuk associated with the long-duration low-luminosity gamma-ray burst (GRB) GRB 171205A at a redshift of 0.037, which is up to now the third GRB-SN event away from us. Our spectroscopic observations and spectral analysis allow us to identify SN 2017iuk as a typical broad-line Type Ic SN. A comparison study suggests that the Type IcBL SN 2017iuk resembles SN 2006aj in the following aspects: (1) similar spectra at the nearby epochs, (2) comparable evolution of the photospheric velocity obtained from the measurements based on both the Si II lambda 6355 line and spectral modeling, and (3) comparable explosion parameters. This analogy could imply the formation of a neutron star in the core collapse of GRB 171205A/SN 2017iuk as previously suggested in GRB 060218/SN 2006aj. The properties of the host galaxy are discussed, which suggest that GRB 171205A/SN 2017iuk occurred in an early-type (S0), high-mass, star-forming galaxy with low specific star formation rate and solar metallicity.
资助项目	National Basic Research Program of China[2014CB845800] ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences[XDA15052600] ; National Natural Science Foundation of China[11533003] ; National Natural Science Foundation of China[11473036] ; National Natural Science Foundation of China[11773036] ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS[XDB23000000] ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS
WOS关键词	GAMMA-RAY BURSTS ; STELLAR SPECTRA ; LIGHT CURVES ; BLACK-HOLES ; GALAXIES ; EXTINCTION ; EMISSION ; STARS ; MODEL ; CLASSIFICATION
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000450221700014
资助机构	National Basic Research Program of China ; National Basic Research Program of China ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS ; National Basic Research Program of China ; National Basic Research Program of China ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS ; National Basic Research Program of China ; National Basic Research Program of China ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS ; National Basic Research Program of China ; National Basic Research Program of China ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; Strategic Pioneer Program on Space Science, Chinese Academy of Sciences ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; One-Hundred-Talent Program of the Chinese Academy of Sciences (CAS) ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Strategic Priority Research Program Multi-wavelength Gravitational Wave Universe of the CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS ; Open Project Program of the Key Laboratory of Optical Astronomy, NAOC, CAS
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/23321]
专题	中国科学院国家天文台
通讯作者	Wang, J.
作者单位	1.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100101, Peoples R China 2.Chinese Acad Sci, Key Lab Space Astron & Technol, Natl Astron Observ, Beijing 100101, Peoples R China 3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China 4.Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Hubei, Peoples R China
推荐引用方式 GB/T 7714	Wang, J.,Zhu, Z. P.,Xu, D.,et al. Spectroscopy of the Type Ic Supernova SN2017iuk Associated with Low-redshift GRB171205A[J]. ASTROPHYSICAL JOURNAL,2018,867(2):7.
APA	Wang, J..,Zhu, Z. P..,Xu, D..,Xin, L. P..,Deng, J. S..,...&Wei, J. Y..(2018).Spectroscopy of the Type Ic Supernova SN2017iuk Associated with Low-redshift GRB171205A.ASTROPHYSICAL JOURNAL,867(2),7.
MLA	Wang, J.,et al."Spectroscopy of the Type Ic Supernova SN2017iuk Associated with Low-redshift GRB171205A".ASTROPHYSICAL JOURNAL 867.2(2018):7.