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Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova

文献类型：期刊论文

作者Xiang, Danfeng1,2; Wang, Xiaofeng1,2; Mo, Jun1,2; Wang, Lingjun3; Smartt, Stephen4; Fraser, Morgan5; Ehgamberdiev, Shuhrat A.6; Mirzaqulov, Davron6; Zhang, Jujia7,8,9; Zhang, Tianmeng10
刊名ASTROPHYSICAL JOURNAL
出版日期2019-02-01
卷号871期号:2页码:20
关键词supernovae: general supernovae: individual (SN 2017ein) stars: Wolf-Rayet
ISSN号0004-637X
DOI10.3847/1538-4357/aaf8b0
英文摘要We present optical and ultraviolet observations of nearby Type Ic supernova (SN Ic) SN 2017ein, as well as a detailed analysis of its progenitor properties from both the early-time observations and the prediscovery Hubble Space Telescope (HST) images. The optical light curves started from within 1 day to similar to 275 days after explosion, and optical spectra range from similar to 2 days to similar to 90 days after explosion. Compared to other normal SNe Ic like SN 2007gr and SN 2013ge, SN 2017ein seems to have more prominent C II absorption and higher expansion velocities in early phases, suggestive of relatively lower ejecta mass. The earliest photometry obtained for SN 2017ein shows indications of shock cooling. The best fit obtained by including a shock-cooling component gives an estimate of the envelope mass as similar to 0.02 M-circle dot and stellar radius as 8 +/- 4 R-circle dot. Examining the pre-explosion images taken with the HST WFPC2, we find that the SN position coincides with a luminous and blue point-like source, with an extinction-corrected absolute magnitude of M-V similar to -8.2 mag and M-I similar to -7.7 mag. Comparisons of the observations to the theoretical models indicate that the counterpart source was either a single W-R star or a binary whose members had high initial masses, or a young compact star cluster. To further distinguish between different scenarios requires revisiting the site of the progenitor with HST after the SN fades away.
WOS关键词GAMMA-RAY BURST ; LIGHT CURVES ; EVOLUTION ; IB ; CONSTRAINTS ; POPULATIONS ; PHOTOMETRY ; GRB-060218 ; HELIUM ; MODELS
资助项目National Natural Science Foundation of China (NSFC)[11178003] ; National Natural Science Foundation of China (NSFC)[11325313] ; National Natural Science Foundation of China (NSFC)[11633002] ; National Program on Key Research and Development Project[2016YFA0400803] ; NSFC[11403096] ; NSFC[11773067] ; NSFC[11203034] ; Key Research Program of the CAS[KJZD-EW-M06] ; Youth Innovation Promotion Association of the CAS[2018081] ; CAS "Light of West China" Program ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; NASA under the Near Earth Objects Observations program (NEOO)[NN12AR55G] ; National Program on Key Research and Development Project of China[2016YFA0400801] ; US National Science Foundation (NSF)[AST-1313484] ; NASA[NNX16AB256] ; Royal Society Science Foundation Ireland University Research Fellowship ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union[GINOP 2.3.2-15-2016-00033] ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS[JP16K17658] ; JSPS[JP26400222] ; JSPS[JP16H02168] ; JSPS[JP17K05382] ; JSPS[JP16H02166] ; [RSF 18-12-00522]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000457281200009
出版者IOP PUBLISHING LTD
资助机构National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; NASA under the Near Earth Objects Observations program (NEOO) ; NASA under the Near Earth Objects Observations program (NEOO) ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; US National Science Foundation (NSF) ; US National Science Foundation (NSF) ; NASA ; NASA ; Royal Society Science Foundation Ireland University Research Fellowship ; Royal Society Science Foundation Ireland University Research Fellowship ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS ; JSPS ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; NASA under the Near Earth Objects Observations program (NEOO) ; NASA under the Near Earth Objects Observations program (NEOO) ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; US National Science Foundation (NSF) ; US National Science Foundation (NSF) ; NASA ; NASA ; Royal Society Science Foundation Ireland University Research Fellowship ; Royal Society Science Foundation Ireland University Research Fellowship ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS ; JSPS ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; NASA under the Near Earth Objects Observations program (NEOO) ; NASA under the Near Earth Objects Observations program (NEOO) ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; US National Science Foundation (NSF) ; US National Science Foundation (NSF) ; NASA ; NASA ; Royal Society Science Foundation Ireland University Research Fellowship ; Royal Society Science Foundation Ireland University Research Fellowship ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS ; JSPS ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Program on Key Research and Development Project ; National Program on Key Research and Development Project ; NSFC ; NSFC ; Key Research Program of the CAS ; Key Research Program of the CAS ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; CAS "Light of West China" Program ; CAS "Light of West China" Program ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; NASA under the Near Earth Objects Observations program (NEOO) ; NASA under the Near Earth Objects Observations program (NEOO) ; National Program on Key Research and Development Project of China ; National Program on Key Research and Development Project of China ; US National Science Foundation (NSF) ; US National Science Foundation (NSF) ; NASA ; NASA ; Royal Society Science Foundation Ireland University Research Fellowship ; Royal Society Science Foundation Ireland University Research Fellowship ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; project "Transient Astrophysical Objects" of the National Research, Development and Innovation Office (NKFIH), Hungary - European Union ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; JSPS ; JSPS
源URL[http://ir.bao.ac.cn/handle/114a11/24945]  
专题中国科学院国家天文台
通讯作者Xiang, Danfeng
作者单位1.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China
2.Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China
3.Chinese Acad Sci, Inst High Energy Phys, Astroparticle Phys, Beijing 100049, Peoples R China
4.Queens Univ Belfast, Sch Math & Phys, Astrophys Res Ctr, Belfast BT7 1NN, Antrim, North Ireland
5.Univ Coll Dublin, Sch Phys, Dublin 4, Ireland
6.Uzbek Acad Sci, Ulugh Beg Astron Inst, Tashkent 100052, Uzbekistan
7.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China
8.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Yunnan, Peoples R China
9.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing 100012, Peoples R China
10.Chinese Acad Sci, Natl Astron Observ China, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714		 Xiang, Danfeng,Wang, Xiaofeng,Mo, Jun,et al. Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova[J]. ASTROPHYSICAL JOURNAL,2019,871(2):20.
APA Xiang, Danfeng.,Wang, Xiaofeng.,Mo, Jun.,Wang, Lingjun.,Smartt, Stephen.,...&Blinnikov, Sergei.(2019).Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova.ASTROPHYSICAL JOURNAL,871(2),20.
MLA Xiang, Danfeng,et al."Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova".ASTROPHYSICAL JOURNAL 871.2(2019):20.

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