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The Red Supergiant Progenitor of the Type II Supernova 2024abfl

文献类型：期刊论文

作者Luo JX(罗竞霄)3,4,5; Zhang LF(张力夫)3,4,5; Chen, Bing-Qiu2; Cheng QY(程其原)3,4,5; Guo BY(郭博洋)3,4,5; Li J(李蛟)3,5; Guo YJ(郭彦君)3,5; Xiong JP(熊建萍)3,5; Meng XC(孟祥存)3,5; Chen XF(陈雪飞)1,3,5
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2025-04-01
卷号982期号:2
ISSN号2041-8205
DOI10.3847/2041-8213/adbf0b
产权排序第1完成单位
文献子类Article
英文摘要Linkage between core-collapse supernovae and their progenitors is not fully understood and ongoing effort of searching and identifying the progenitors is needed. SN 2024abfl is a recent Type II supernova that exploded in the nearby star-bursting galaxy NGC 2146, which is also the host galaxy of SN 2018zd. From archival Hubble Space Telescope data, we have found a red source (mF814W similar to 25) near the location (angular distance <= 0 .'' 2) of SN 2024abfl before its explosion. With F814W and F606W photometry, we found that the properties of this source matched a typical red supergiant (RSG) moderately reddened by interstellar dust at the distance of the host galaxy. We conclude that the SN 2024abfl had an RSG progenitor with initial mass of 9 -12 M circle dot.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词ELECTRON-CAPTURE SUPERNOVAE ; MESA ISOCHRONES ; MASSIVE SINGLE ; SN 2023IXF ; STARS ; EVOLUTION ; EXPLOSION ; MODULES ; ABSORPTION ; ASTROPY
资助项目National Natural Science Foundation of China (NSFC)[12288102]; National Natural Science Foundation of China (NSFC)[12125303]; National Natural Science Foundation of China (NSFC)[12090040/1]; National Natural Science Foundation of China (NSFC)[11873016]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB1160303]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB1160300]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB1160000]; National Key R&D Program of China[2021YFA1600401]; National Key R&D Program of China[2021YFA1600400]; Chinese Academy of Sciences (CAS); International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001]; Yunnan Fundamental Research Projects[202305AB350003]; Yunnan Fundamental Research Projects[202001AW070007]; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202401CF070035]; Yunnan Fundamental Research Projects (YFRP)[202401CF070035]; Young Talent Project of Yunnan Revitalization Talent Support Program
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001456043300001
出版者IOP Publishing Ltd
资助机构National Natural Science Foundation of China (NSFC)[12288102, 12125303, 12090040/1, 11873016] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB1160303, XDB1160300, XDB1160000] ; National Key R&D Program of China[2021YFA1600401, 2021YFA1600400] ; Chinese Academy of Sciences (CAS) ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001] ; Yunnan Fundamental Research Projects[202305AB350003, 202001AW070007] ; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202401CF070035] ; Yunnan Fundamental Research Projects (YFRP)[202401CF070035] ; Young Talent Project of Yunnan Revitalization Talent Support Program
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28246]  
专题云南天文台_大样本恒星演化研究组
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, CAS, Kunming 650216, People's Republic of China
2.South-Western Institute for Astronomy Research, Yunnan University, Kunming 650500, People's Republic of China;
3.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China;
4.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
5.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People's Republic of China; cxf@ynao.ac.cn, zwliu@ynao.ac.cn;
推荐引用方式
GB/T 7714		 Luo JX,Zhang LF,Chen, Bing-Qiu,et al. The Red Supergiant Progenitor of the Type II Supernova 2024abfl[J]. ASTROPHYSICAL JOURNAL LETTERS,2025,982(2).
APA 罗竞霄.,张力夫.,Chen, Bing-Qiu.,程其原.,郭博洋.,...&韩占文.(2025).The Red Supergiant Progenitor of the Type II Supernova 2024abfl.ASTROPHYSICAL JOURNAL LETTERS,982(2).
MLA 罗竞霄,et al."The Red Supergiant Progenitor of the Type II Supernova 2024abfl".ASTROPHYSICAL JOURNAL LETTERS 982.2(2025).

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来源：云南天文台

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