中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Circumstellar material ejected violently by a massive star immediately before its death

文献类型:期刊论文

作者Zhang JJ(张居甲)1,7,8; Lin H(林含)1,6,8; Wang, Xiaofeng4,5; Zhao ZY(赵泽毅)1,7,8; Li LP(李丽萍)8; Liu, Jialian5; Yan, Shengyu5; Xiang, Danfeng5; Wang, Huijuan2,3; Bai JM(白金明)1,7,8
刊名SCIENCE BULLETIN
出版日期2023-11-15
卷号68期号:21页码:2548-2554
关键词Supernova: SN 2023ixf Core -collapse supernova Circumstellar material Mass loss
ISSN号2095-9273
DOI10.1016/j.scib.2023.09.015
产权排序第1完成单位
文献子类Article
英文摘要Type II supernovae represent the most common stellar explosions in the Universe, for which the final stage evolution of their hydrogen-rich massive progenitors towards core-collapse explosion are elusive. The recent explosion of SN 2023ixf in a very nearby galaxy, Messier 101, provides a rare opportunity to explore this longstanding issue. With the timely high-cadence flash spectra taken within 1-5 days after the explosion, we can put stringent constraints on the properties of the surrounding circumstellar material around this supernova. Based on the rapid fading of the narrow emission lines and luminosity/profile of H alpha emission at very early times, we estimate that the progenitor of SN 2023ixf lost material at a mass-loss rate M-center dot approximate to 6x10(-4)M(circle dot)a(-1) over the last 2-3 years before explosion. This close-by material, moving at a velocity v(w)approximate to 55kms(-1), accumulates a compact CSM shell at the radius smaller than 7x10(14) cm from the progenitor. Given the high mass-loss rate and relatively large wind velocity presented here, together with the pre-explosion observations made about two decades ago, the progenitor of SN 2023ixf could be a short-lived yellow hypergiant that evolved from a red supergiant shortly before the explosion.
学科主题天文学
URL标识查看原文
出版地RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
WOS关键词SN 1999EM ; ENVIRONMENT ; EVOLUTION ; DISTANCE
资助项目National Key R&D Program of China[2021YFA1600404]; National Natural Science Foundation of China; China Manned Space Project[12173082]; China Manned Space Project[CMS-CSST-2021-A12]; China Manned Space Project[202201AT070069]; China Manned Space Project[202302AN360001]; Yunnan Province Foundation[12288102]; Top-notch Young Talents Program of Yunnan Province[12033003]; Chinese Academy of Sciences; International Centre of Supernovae, Yunnan Key Laboratory; Scholar Program of Beijing Academy of Science and Technology[11633002]; Tencent Xplorer Prize[DZ:BS202002]; CAS; People's Government of Yunnan Province
WOS研究方向Science & Technology - Other Topics
语种英语
WOS记录号WOS:001114484100001
出版者ELSEVIER
资助机构National Key R&D Program of China[2021YFA1600404] ; National Natural Science Foundation of China ; China Manned Space Project[12173082, CMS-CSST-2021-A12, 202201AT070069, 202302AN360001] ; Yunnan Province Foundation[12288102] ; Top-notch Young Talents Program of Yunnan Province[12033003] ; Chinese Academy of Sciences ; International Centre of Supernovae, Yunnan Key Laboratory ; Scholar Program of Beijing Academy of Science and Technology[11633002] ; Tencent Xplorer Prize[DZ:BS202002] ; CAS ; People's Government of Yunnan Province
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/26515]  
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
作者单位1.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China;
2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 101408, China
3.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;
4.Beijing Planetarium, Beijing Academy of Science and Technology, Beijing 100044, China;
5.Department of Physics, Tsinghua University, Beijing 100084, China;
6.Key Laboratory of Radio Astronomy and Technology, CAS, Beijing 100101, China;
7.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, China;
8.Yunnan Observatories (YNAO), Chinese Academy of Sciences, Kunming 650216, China;
推荐引用方式
GB/T 7714
Zhang JJ,Lin H,Wang, Xiaofeng,et al. Circumstellar material ejected violently by a massive star immediately before its death[J]. SCIENCE BULLETIN,2023,68(21):2548-2554.
APA 张居甲.,林含.,Wang, Xiaofeng.,赵泽毅.,李丽萍.,...&白金明.(2023).Circumstellar material ejected violently by a massive star immediately before its death.SCIENCE BULLETIN,68(21),2548-2554.
MLA 张居甲,et al."Circumstellar material ejected violently by a massive star immediately before its death".SCIENCE BULLETIN 68.21(2023):2548-2554.

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