Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
文献类型:期刊论文
作者 | Bostroem, K. A.1; Valenti, S.1; Sand, D. J.2; Andrews ,J. E.2; Van Dyk, S. D.3; Galbany, L.4; Pooley, D.5,6; Amaro, R. C.2; Smith, N.2; Yang, S.1,7,8 |
刊名 | ASTROPHYSICAL JOURNAL |
出版日期 | 2020-05-01 |
卷号 | 895期号:1页码:20 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/ab8945 |
产权排序 | 第34完成单位 |
文献子类 | Article |
英文摘要 | We present the discovery and high-cadence follow-up observations of SN 2018ivc, an unusual SNe II that exploded in NGC 1068 (D = 10.1 Mpc). The light curve of SN 2018ivc declines piecewise-linearly, changing slope frequently, with four clear slope changes in the first 30 days of evolution. This rapidly changing light curve indicates that interaction between the circumstellar material and ejecta plays a significant role in the evolution. Circumstellar interaction is further supported by a strong X-ray detection. The spectra are rapidly evolving and dominated by hydrogen, helium, and calcium emission lines. We identify a rare high-velocity emission-line feature blueshifted at similar to 7800 (in H alpha, H beta, P beta, P gamma, He i, and Ca ii), which is visible from day 18 until at least day 78 and could be evidence of an asymmetric progenitor or explosion. From the overall similarity between SN 2018ivc and SN 1996al, the H alpha equivalent width of its parent H ii region, and constraints from pre-explosion archival Hubble Space Telescope images, we find that the progenitor of SN 2018ivc could be as massive as 52 but is more likely <12. SN 2018ivc demonstrates the importance of the early discovery and rapid follow-up observations of nearby supernovae to study the physics and progenitors of these cosmic explosions. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星天文学 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | RED SUPERGIANT PROGENITOR ; LIGHT CURVES ; CIRCUMSTELLAR INTERACTION ; STELLAR POPULATIONS ; P SUPERNOVAE ; MASS-LOSS ; EVOLUTION ; STAR ; LUMINOSITY ; TELESCOPE |
资助项目 | NSF[AST-1813176] ; NSF[AST-1821967] ; NSF[1821987] ; NSF[1813708] ; NSF[1813466] ; NSF[1908972] ; NSF[AST-151559] ; NSF[AST-1313484] ; NSF[AST-1813825] ; European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant[839090] ; Israel Science Foundation[2108/18] ; Israel Science Foundation[2752/19] ; United States-Israel Binational Science Foundation (BSF) ; Israeli Council for Higher Education Alon Fellowship ; Christopher R. Redlich Fund ; TABASGO Foundation ; Miller Institute for Basic Research in Science (UC Berkeley) ; Department of Science and Technology (DST), Government of India ; Indo-US Science and Technology Forum (IUSSTF) ; NASA ADAP[NNX13AF35G] ; NASA ADAP[NNX17AF43G] ; National Aeronautics and Space Administration (NASA) through Chandra Award[GO8-19051X] ; NASA[NAS8-03060] ; NASA[NNX16AB25G] ; NASA[NAS 5-26555] ; National Natural Science Foundation of China (NSFC)[11773067] ; National Natural Science Foundation of China (NSFC)[11403096] ; National Natural Science Foundation of China (NSFC)[11325313] ; National Natural Science Foundation of China (NSFC)[11633002] ; Youth Innovation Promotion Association of the CAS[2018081] ; Western Light Youth Project ; National Program on Key Research and Development Project[2016YFA0400803] ; 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 ; Gemini Observatory[GS-2018B-Q-130] ; NASA through a STScI[GO-15151] ; W. M. Keck Foundation |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000536905500001 |
资助机构 | NSF[AST-1813176, AST-1821967, 1821987, 1813708, 1813466, 1908972, AST-151559, AST-1313484, AST-1813825] ; European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant[839090] ; Israel Science Foundation[2108/18, 2752/19] ; United States-Israel Binational Science Foundation (BSF) ; Israeli Council for Higher Education Alon Fellowship ; Christopher R. Redlich Fund ; TABASGO Foundation ; Miller Institute for Basic Research in Science (UC Berkeley) ; Department of Science and Technology (DST), Government of India ; Indo-US Science and Technology Forum (IUSSTF) ; NASA ADAP[NNX13AF35G, NNX17AF43G] ; National Aeronautics and Space Administration (NASA) through Chandra Award[GO8-19051X] ; NASA[NAS8-03060, NNX16AB25G, NAS 5-26555] ; National Natural Science Foundation of China (NSFC)[11773067, 11403096, 11325313, 11633002] ; Youth Innovation Promotion Association of the CAS[2018081] ; Western Light Youth Project ; National Program on Key Research and Development Project[2016YFA0400803] ; 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 ; Gemini Observatory[GS-2018B-Q-130] ; NASA through a STScI[GO-15151] ; W. M. Keck Foundation |
源URL | [http://ir.ynao.ac.cn/handle/114a53/23287] |
专题 | 云南天文台_丽江天文观测站(南方基地) 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Bostroem, K. A. |
作者单位 | 1.Department of Physics, University of California, 1 Shields Avenue, Davis, CA 95616-5270, USA 2.Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA 3.Caltech/IPAC, Mailcode 100-22, Pasadena, CA 91125, USA 4.Departamento de Fsica Terica y del Cosmos, Universidad de Granada, E-18071 Granada, Spain 5.Department of Physics and Astronomy, Trinity University, San Antonio TX, USA 6.Eureka Scientific, Inc., USA 7.Department of Physics and Astronomy Galileo Galilei, University of Padova, Vicolo dell’Osservatorio, 3, I-35122 Padova, Italy 8.INAF—Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy 9.Indian Institute of Astrophysics, Koramangala 2nd Block, Bengaluru 560 034, India 10.The School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel |
推荐引用方式 GB/T 7714 | Bostroem, K. A.,Valenti, S.,Sand, D. J.,et al. Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068[J]. ASTROPHYSICAL JOURNAL,2020,895(1):20. |
APA | Bostroem, K. A..,Valenti, S..,Sand, D. J..,Andrews ,J. E..,Van Dyk, S. D..,...&Zhang, X..(2020).Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068.ASTROPHYSICAL JOURNAL,895(1),20. |
MLA | Bostroem, K. A.,et al."Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068".ASTROPHYSICAL JOURNAL 895.1(2020):20. |
入库方式: OAI收割
来源:云南天文台
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