SN 2016coi/ASASSN-16fp: an example of residual helium in a type Ic supernova?
文献类型：期刊论文
| 作者 | Prentice, S. J.1; Ashall, C.1,2; Mazzali, P. A.1,3; Zhang, J. -J.4,5,6; James, P. A.1; Wang, X. -F.7,8; Vinko, J.9,10,11; Percival, S.1; Short, L.1; Piascik, A.1 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 出版日期 | 2018-08-01 |
| 卷号 | 478期号:3页码:4162-4192 |
| ISSN号 | 0035-8711 |
| 关键词 | supernovae: individual SN2016coi/ASASSN16-fp |
| DOI | 10.1093/mnras/sty1223 |
| 英文摘要 | The optical observations of Ic-4 supernova (SN) 2016coi/ASASSN-16fp, from similar to 2 to similar to 450 d after explosion, are presented along with analysis of its physical properties. The SN shows the broad lines associated with SNe Ic-3/4 but with a key difference. The early spectra display a strong absorption feature at similar to 5400 angstrom which is not seen in other SNe Ic-3/4 at this epoch. This feature has been attributed to He I in the literature. Spectral modelling of the SN in the early photospheric phase suggests the presence of residual He in a C/O dominated shell. However, the behaviour of the He I lines is unusual when compared with He-rich SNe, showing relatively low velocities and weakening rather than strengthening over time. The SN is found to rise to peak similar to 16 d after core-collapse reaching a bolometric luminosity of L-p similar to 3 x 10(42) erg s(-1). Spectral models, including the nebular epoch, show that the SN ejected 2.5-4M(circle dot) of material, with similar to 1.5M(circle dot) below 5000 km s(-1), and with a kinetic energy of (4.5-7) x 10(51) erg. The explosion synthesized similar to 0.14M(circle dot) of Ni-56. There are significant uncertainties in E(B - V)(host) and the distance, however, which will affect L-p and M-Ni. SN 2016coi exploded in a host similar to the Large Magellanic Cloud (LMC) and away from star-forming regions. The properties of the SN and the host-galaxy suggest that the progenitor had M-ZAMS of 23-28M(circle dot) and was stripped almost entirely down to its C/O core at explosion. |
| WOS关键词 | STRIPPED-ENVELOPE SUPERNOVAE ; CORE-COLLAPSE SUPERNOVAE ; NEBULAR SPECTRA ; IIB SUPERNOVA ; PRESUPERNOVA EVOLUTION ; PHOTOMETRIC SYSTEM ; BINARY COMPANION ; STAR-FORMATION ; LIGHT CURVES ; TELESCOPE |
| 资助项目 | Science and Technology Facilities Council (STFC) ; National Science Foundation (NSF)[AST-1613472] ; STFC ; NSF[1313484] ; NSF[AST-1412504] ; NSF[AST-1517649] ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; National Science Foundation of China (NSFC)[11403096] ; National Science Foundation of China (NSFC)[11773067] ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Key Research Program of the CAS[KJZD-EW-M06] |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| 出版者 | OXFORD UNIV PRESS |
| WOS记录号 | WOS:000441282300093 |
| 资助机构 | Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; STFC ; STFC ; NSF ; NSF ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Key Research Program of the CAS ; Key Research Program of the CAS ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; STFC ; STFC ; NSF ; NSF ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Key Research Program of the CAS ; Key Research Program of the CAS ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; STFC ; STFC ; NSF ; NSF ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Key Research Program of the CAS ; Key Research Program of the CAS ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; STFC ; STFC ; NSF ; NSF ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province ; People's Government of Yunnan Province ; National Science Foundation of China (NSFC) ; National Science Foundation of China (NSFC) ; Youth Innovation Promotion Association of the CAS ; Youth Innovation Promotion Association of the CAS ; Western Light Youth Project ; Western Light Youth Project ; Key Research Program of the CAS ; Key Research Program of the CAS |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/22533]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Prentice, S. J.; Ashall, C. |
| 作者单位 | 1.Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England 2.Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA 3.Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany 4.Chinese Acad Sci, Yunnan Observ YNAO, Kunming 650216, Yunnan, Peoples R China 5.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Yunnan, Peoples R China 6.Chinese Acad Sci, Ctr Astron Mega Sci, 20A Datun Rd, Beijing 100012, Peoples R China 7.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China 8.Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China 9.Konkoly Observ Budapest, Res Ctr Astron & Earth Sci, Konkoly Thege Ut 15-17, H-1121 Budapest, Hungary 10.Univ Szeged, Dept Opt & Quantum Elect, Dom Ter 9, H-6720 Szeged, Hungary |
| 推荐引用方式 GB/T 7714 | Prentice, S. J.,Ashall, C.,Mazzali, P. A.,et al. SN 2016coi/ASASSN-16fp: an example of residual helium in a type Ic supernova?[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,478(3):4162-4192. |
| APA | Prentice, S. J..,Ashall, C..,Mazzali, P. A..,Zhang, J. -J..,James, P. A..,...&Tartaglia, L..(2018).SN 2016coi/ASASSN-16fp: an example of residual helium in a type Ic supernova?.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,478(3),4162-4192. |
| MLA | Prentice, S. J.,et al."SN 2016coi/ASASSN-16fp: an example of residual helium in a type Ic supernova?".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 478.3(2018):4162-4192. |
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来源：国家天文台
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