| The dusty and extremely red progenitor of the type II supernova 2023ixf in Messier 101 | |
Xiang, Danfeng1; Mo, Jun1; Wang, Lingzhi2; Wang, Xiaofeng1,3; Zhang JJ(张居甲)4,5,6 ; Lin H(林含)4,5; Wang, Lifan7
| |
| 发表期刊 | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
 |
| 2024-01 | |
| 卷号 | 67期号:1 |
| DOI | 10.1007/s11433-023-2267-0 |
| 产权排序 | 第4完成单位 |
| 收录类别 | SCI ; EI |
| 关键词 | stellar evolution mass loss red supergiants infrared emission supernovae |
| 摘要 | Stars with initial masses in the range of 8-25 solar masses are thought to end their lives as hydrogen-rich supernovae (SNe II). Based on the pre-explosion images of Hubble space telescope (HST) and Spitzer space telescope, we place tight constraints on the progenitor candidate of type IIP SN 2023ixf in Messier 101. Fitting of the spectral energy distribution (SED) of its progenitor with dusty stellar spectral models results in an estimation of the effective temperature as 3091-258+422 K. The luminosity is estimated as lg(L/L circle dot)similar to 4.83, consistent with a red supergiant (RSG) star with an initial mass of 12-1+2M circle dot. The derived mass loss rate (6x10-6-9x10-6M circle dot yr-1) is much lower than that inferred from the flash spectroscopy of the SN, suggesting that the progenitor experienced a sudden increase in mass loss when approaching the final explosion. In the infrared bands, significant deviation from the range of regular RSGs in the color-magnitude diagram and period-luminosity space of the progenitor star indicates enhanced mass loss and dust formation. Combined with new evidence of polarization at the early phases of SN 2023ixf, such a violent mass loss is likely a result of binary interaction. |
| 资助项目 | National Natural Science Foundation of China[12288102]; National Natural Science Foundation of China[12033003]; National Natural Science Foundation of China[11633002]; Ma Huateng Foundation; Scholar Program of Beijing Academy of Science and Technology[DZ:BS202002]; Tencent Xplorer Prize; Chinese Academy of Sciences (CAS); People's Government of Yunnan Province |
| 项目资助者 | National Natural Science Foundation of China[12288102, 12033003, 11633002] ; Ma Huateng Foundation ; Scholar Program of Beijing Academy of Science and Technology[DZ:BS202002] ; Tencent Xplorer Prize ; Chinese Academy of Sciences (CAS) ; People's Government of Yunnan Province |
| 语种 | 英语 |
| 学科领域 | 天文学 |
| 文章类型 | Article |
| 出版者 | SCIENCE PRESS |
| 出版地 | 16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA |
| ISSN | 1674-7348 |
| URL | 查看原文 |
| WOS记录号 | WOS:001127209200001 |
| WOS研究方向 | Physics |
| WOS类目 | Physics, Multidisciplinary |
| 关键词[WOS] | ELECTRON-CAPTURE SUPERNOVAE ; PERIOD-LUMINOSITY RELATIONS ; MARCS MODEL ATMOSPHERES ; MASSIVE STARS ; CORE-COLLAPSE ; SN 2023IXF ; MESA ISOCHRONES ; AGB STARS ; EVOLUTION ; SUPERGIANT |
| EI入藏号 | 20235115259756 |
| EI主题词 | Luminance |
| EI分类号 | 615.2 Solar Power - 657.2 Extraterrestrial Physics and Stellar Phenomena - 741.3 Optical Devices and Systems |
| 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/114a53/26511 |
| 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.Department of Physics, Tsinghua University, Beijing, 100084, China; 2.South America Center for Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China; 3.Beijing Planetarium, Beijing Academy of Sciences and Technology, Beijing, 100044, China; 4.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China; 5.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650216, China; 6.International Centre of Supernovae, Yunnan Key Laboratory, Kunming, 650216, China; 7.Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University, College Station, TX, 77843, USA |
| 推荐引用方式 GB/T 7714 | Xiang, Danfeng,Mo, Jun,Wang, Lingzhi,et al. The dusty and extremely red progenitor of the type II supernova 2023ixf in Messier 101[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2024,67(1). |
| APA | Xiang, Danfeng.,Mo, Jun.,Wang, Lingzhi.,Wang, Xiaofeng.,张居甲.,...&Wang, Lifan.(2024).The dusty and extremely red progenitor of the type II supernova 2023ixf in Messier 101.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,67(1). |
| MLA | Xiang, Danfeng,et al."The dusty and extremely red progenitor of the type II supernova 2023ixf in Messier 101".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 67.1(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 | ||
| The dusty and extrem（2832KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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。
修改评论