中文版 | English
YNAO OpenIR  > 南方基地
Early-time Observations of SN 2023wrk: A Luminous Type Ia Supernova with Significant Unburned Carbon in the Outer Ejecta
Liu, Jialian1; Wang, Xiaofeng1; Andrade, Cristina2; Duverne, Pierre-Alexandre3; Zhang JJ(张居甲)4,5,6; Li LP(李丽萍)4,5,6; Wang ZY(王振宇)4,5,6,7; Navarete, Felipe8; Reguitti, Andrea9,10; Schuldt, Stefan11,12; Cai YZ(蔡永志)4,5,6; Filippenko, Alexei V.13; Yang, Yi1,13; Brink, Thomas G.13; Zheng, WeiKang13; Esamdin, Ali14; Iskandar, Abdusamatjan14,15; Bai, Chunhai14; Liu, Jinzhong14; Li, Xin16; Hu, Maokai1; Li, Gaici1; Li, Wenxiong17; Ma, Xiaoran1; Yan, Shengyu1; Mo, Jun1; Adami, Christophe18; Akl, Dalya19; Antier, Sarah20; Broens, Eric21; Ducoin, Jean-Grégoire22; Elhosseiny, Eslam23; Esposito, Thomas M.13; Freeberg, Michael24,25; Gokuldass, Priyadarshini26; Hello, Patrice27; Karpov, Sergey28; Márquez, Isabel29; Mašek, Martin30; Pyshna, Oleksandra31; Rajabov, Yodgor32; Saint-Gelais, Denis33; Serrau, Marc34; Sokoliuk, Oleksii35,36; Takey, Ali23; Tanasan, Manasanun37; Turpin, Damien38
发表期刊ASTROPHYSICAL JOURNAL
2024-10-01
卷号973期号:2
DOI10.3847/1538-4357/ad6600
产权排序第4完成单位
收录类别SCI
摘要We present extensive photometric and spectroscopic observations of the nearby Type Ia supernova (SN) 2023wrk at a distance of about 40 Mpc. The earliest detection of this SN can be traced back to a few hours after the explosion. Within the first few days, the light curve shows a bump feature, while the B - V color is blue and remains nearly constant. The overall spectral evolution is similar to that of an SN 1991T/SN 1999aa-like SN Ia, while the C ii lambda 6580 absorption line appears to be unusually strong in the first spectrum taken at t approximate to -15.4 days after the maximum light. This carbon feature disappears quickly in subsequent evolution but it reappears at around the time of peak brightness. The complex evolution of the carbon line and the possible detection of Ni iii absorption around 4700 & Aring; and 5300 & Aring; in the earliest spectra indicate macroscopic mixing of fuel and ash. The strong carbon lines are likely related to the collision of SN ejecta with unbound carbon, consistent with the predictions of pulsational delayed-detonation or carbon-rich circumstellar-matter interaction models. Among those carbon-rich SNe Ia with strong C ii lambda 6580 absorption at very early times, the line-strength ratio of C ii to Si ii and the B - V color evolution are found to exhibit large diversity, which may be attributed to different properties of unbound carbon and outward-mixing 56Ni.
资助项目National Natural Science Foundation of China (NSFC)[12288102]; National Natural Science Foundation of China (NSFC)[12033003]; National Natural Science Foundation of China (NSFC)[12090044]; Tencent Xplorer Prize; Tianshan Talent Training Program[2023TSYCCX0101]; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001]; National Key R&D Program of China[2021YFA1600404]; NSFC[12173082]; NSFC[12303054]; Yunnan Province Foundation[202201AT070069]; Top-notch Young Talents Program of Yunnan Province; Light of West China Program by the Chinese Academy of Sciences; NOIRLab[202401AU070063]; Yunnan Fundamental Research Projects; Laboratorio Nacional de Astrofisica (LNA) from OPD; Christopher R. Redlich Fund; Universidade do Estado do Amazonas-UEA and LNA[24CD013]; Innovation Project of Being Academy of Science and Technology; CNRS-MITI and Programme National des Hautes Energies (PNHE); GRAWITA Large Program Grant; W. M. Keck Foundation; PRIN-INAF 2022 program; Tianshan Talent Training Program[CEX2021-001131-S]; Severo Ochoa grant - MCIN/AEI; National Key R&D program of China for Intergovernmental Scientific and Technological Innovation Cooperation Project; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[P-003]; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[P-011]; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[I-004]; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[I-013]; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[I-009]; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[I-022]; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[I-027]; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[P-008]; Thai Robotic Telescope[P-003]; Thai Robotic Telescope[I-004]; Thai Robotic Telescope[P-008]; Thai Robotic Telescope[I-007]; Heising-Simons Foundation; NASA; Ministry of Education of the Czech Republic[2023TSYCLJ0053]; EU/MEYS[2022YFE0126200]; Egyptian Science, Technology & Innovation Funding Authority (STDF); Observatoire de Haute-Provence[TRTToO_2024001]; Observatoire de Haute-Provence[TRTC11B_002]; Thai Robotic Telescope
项目资助者National Natural Science Foundation of China (NSFC)[12288102, 12033003, 12090044] ; Tencent Xplorer Prize ; Tianshan Talent Training Program[2023TSYCCX0101] ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001] ; National Key R&D Program of China[2021YFA1600404] ; NSFC[12173082, 12303054] ; Yunnan Province Foundation[202201AT070069] ; Top-notch Young Talents Program of Yunnan Province ; Light of West China Program by the Chinese Academy of Sciences ; NOIRLab[202401AU070063] ; Yunnan Fundamental Research Projects ; Laboratorio Nacional de Astrofisica (LNA) from OPD ; Christopher R. Redlich Fund ; Universidade do Estado do Amazonas-UEA and LNA[24CD013] ; Innovation Project of Being Academy of Science and Technology ; CNRS-MITI and Programme National des Hautes Energies (PNHE) ; GRAWITA Large Program Grant ; W. M. Keck Foundation ; PRIN-INAF 2022 program ; Tianshan Talent Training Program[CEX2021-001131-S] ; Severo Ochoa grant - MCIN/AEI ; National Key R&D program of China for Intergovernmental Scientific and Technological Innovation Cooperation Project ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences[P-003, P-011, I-004, I-013, I-009, I-022, I-027, P-008] ; Thai Robotic Telescope[P-003, I-004, P-008, I-007] ; Heising-Simons Foundation ; NASA ; Ministry of Education of the Czech Republic[2023TSYCLJ0053] ; EU/MEYS[2022YFE0126200] ; Egyptian Science, Technology & Innovation Funding Authority (STDF) ; Observatoire de Haute-Provence[TRTToO_2024001, TRTC11B_002] ; Thai Robotic Telescope[12540303] ; [LM2023032] ; [LM2023047] ; [CZ.02.1.01/0.0/0.0/16_013/0001403] ; [CZ.02.1.01/0.0/0.0/18_046/0016007] ; [CZ.02.1.01/0.0/0.0/16_019/0000754] ; [CZ.02.01.01/00/22_008/0004632] ; [45779] ; [TRTC11A_003]
语种英语
学科领域天文学
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001320973300001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]HUBBLE-SPACE-TELESCOPE ; NEAR-INFRARED OBSERVATIONS ; EARLY EXCESS EMISSION ; LIGHT CURVES ; DATA RELEASE ; ABUNDANCE STRATIFICATION ; ABSOLUTE MAGNITUDES ; PHOTOMETRIC SYSTEM ; OPTICAL-SPECTRA ; LOCAL VALUE
引用统计
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/27622
专题南方基地
中国科学院天体结构与演化重点实验室
作者单位1.Physics Department, Tsinghua University, Beijing 100084, People's Republic of China; [email protected], [email protected];
2.School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA;
3.Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France;
4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
5.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China;
6.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
7.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
8.SOAR Telescope/NSF's NOIRLab Avda Juan Cisternas 1500, 1700000 La Serena, Chile;
9.INAF—Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate (LC), Italy;
10.INAF—Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy;
11.Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, I-20133 Milano, Italy;
12.INAF—IASF Milano, via A. Corti 12, I-20133 Milano, Italy;
13.Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA;
14.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, People's Republic of China;
15.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
16.Beijing Planetarium, Beijing Academy of Science and Technology, Beijing 100044, People's Republic of China;
17.Natioal Astronomical Observatories of China, Chinese Academy of Sciences, Beijing 100012, People's Republic of China;
18.Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France;
19.Physics Department, American University of Sharjah, Sharjah, UAE;
20.Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire J.-L. Lagrange, Boulevard de l'Observatoire, 06304 Nice, France;
21.KNC, Vereniging Voor Sterrenkunde, Balen-Neetlaan 18A, B-2400 Mol, Belgium;
22.CPPM, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France;
23.National Research Institute of Astronomy and Geophysics (NRIAG), 1 El-marsad St., 11421 Helwan, Cairo, Egypt;
24.KNC, AAVSO, Hidden Valley Observatory (HVO), Colfax, WI 54730, USA;
25.iTelescope, Utah Desert Remote Observatory, Beryl Junction, UT 84714, USA;
26.Department of Physical Sciences, College of Arts and Sciences, Embry-Riddle Aeronautical University, Daytona Beach, FL 32114, USA;
27.IJCLab, Univ Paris-Saclay, CNRS/IN2P3, Orsay, France;
28.CEICO, Institute of Physics of the Czech Academy of Sciences, Na Slovance 1999/2, CZ-182 21 Praha, Czech Republic;
29.Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía, 18008 Granada, Spain;
30.FZU—Institute of Physics, Czech Academy of Sciences, Na Slovance 1999/2, CZ-182 21 Praha, Czech Republic;
31.The Astronomical observatory of Taras Shevchenko National University of Kyiv, Ukraine;
32.Ulugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, Astronomy Str. 33, Tashkent 100052, Uzbekistan;
33.KNC, Sociedad Astronomica Queretana, Mexico, RAPAS Observatoire de Paris, France, Le club des Astronome Amateur de Rosemère du Québec, Canada;
34.KNC, Société Astronomique de France, Observatoire de Dauban, F-04150 Banon, France;
35.Astronomical Observatory of Taras Shevchenko National University of Kyiv, Observatorna Str. 3, Kyiv, 04053, Ukraine;
36.Main Astronomical Observatory of National Academy of Sciences of Ukraine, 27 Acad. Zabolotnoho Str., Kyiv 03143, Ukraine;
37.National Astronomical Research Institute of Thailand (Public Organization), 260, Moo 4, T. Donkaew, A. Mae Rim, Chiang Mai 50180, Thailand;
38.Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191 Gif-sur-Yvette, France
推荐引用方式
GB/T 7714		 Liu, Jialian,Wang, Xiaofeng,Andrade, Cristina,et al. Early-time Observations of SN 2023wrk: A Luminous Type Ia Supernova with Significant Unburned Carbon in the Outer Ejecta[J]. ASTROPHYSICAL JOURNAL,2024,973(2).
APA Liu, Jialian.,Wang, Xiaofeng.,Andrade, Cristina.,Duverne, Pierre-Alexandre.,张居甲.,...&Turpin, Damien.(2024).Early-time Observations of SN 2023wrk: A Luminous Type Ia Supernova with Significant Unburned Carbon in the Outer Ejecta.ASTROPHYSICAL JOURNAL,973(2).
MLA Liu, Jialian,et al."Early-time Observations of SN 2023wrk: A Luminous Type Ia Supernova with Significant Unburned Carbon in the Outer Ejecta".ASTROPHYSICAL JOURNAL 973.2(2024).
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
Early-time Observati（4528KB）期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Liu, Jialian]的文章
[Wang, Xiaofeng]的文章
[Andrade, Cristina]的文章
百度学术
百度学术中相似的文章
[Liu, Jialian]的文章
[Wang, Xiaofeng]的文章
[Andrade, Cristina]的文章
必应学术
必应学术中相似的文章
[Liu, Jialian]的文章
[Wang, Xiaofeng]的文章
[Andrade, Cristina]的文章
相关权益政策
暂无数据
收藏/分享
文件名： Early-time Observations of SN 2023wrk_ A Luminous Type Ia Supernova with Significant Unburned Carbon in the Outer Ejecta.pdf
格式： Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。