The Red Supergiant Progenitor of the Type II Supernova 2024abfl

doi:10.3847/2041-8213/adbf0b

YNAO OpenIR > 大样本恒星演化研究组

	The Red Supergiant Progenitor of the Type II Supernova 2024abfl
	Luo JX(罗竞霄)1,2,3 ; Zhang LF(张力夫)1,2,3 ; Chen, Bing-Qiu 4; Cheng QY(程其原)1,2,3 ; Guo BY(郭博洋)1,2,3 ; Li J(李蛟)1,3 ; Guo YJ(郭彦君)1,3 ; Xiong JP(熊建萍)1,3 ; Meng XC(孟祥存)1,3 ; Chen XF(陈雪飞)1,3,5 ; Liu ZW(柳正伟)1,3 ; Han ZW(韩占文)1,3,5
发表期刊	ASTROPHYSICAL JOURNAL LETTERS
	2025-04-01
卷号	982 期号:2
DOI	10.3847/2041-8213/adbf0b
产权排序	第1完成单位
收录类别	SCI
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.
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
项目资助者	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
语种	英语
学科领域	天文学 ; 恒星与银河系
文章类型	Article
出版者	IOP Publishing Ltd
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN	2041-8205
URL	查看原文
WOS记录号	WOS:001456043300001
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	ELECTRON-CAPTURE SUPERNOVAE ; MESA ISOCHRONES ; MASSIVE SINGLE ; SN 2023IXF ; STARS ; EVOLUTION ; EXPLOSION ; MODULES ; ABSORPTION ; ASTROPY
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/114a53/28246
专题	大样本恒星演化研究组中国科学院天体结构与演化重点实验室
作者单位	1.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People's Republic of China; [email protected], [email protected]; 2.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China; 3.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China; 4.South-Western Institute for Astronomy Research, Yunnan University, Kunming 650500, People's Republic of China; 5.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650216, People's Republic of China
第一作者单位	中国科学院云南天文台
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).

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
The Red Supergiant P（1038KB）	期刊论文	出版稿	开放获取	CC BY-NC-SA	浏览请求全文