| Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars | |
Luo JX(罗竞霄)1,2,3,4 ; Dessart, Luc5; Chen XF(陈雪飞)1,2,4; Liu ZW(柳正伟)1,2,4
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| 发表期刊 | ASTRONOMY & ASTROPHYSICS
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| 2024-09-17 | |
| 卷号 | 689 |
| DOI | 10.1051/0004-6361/202349123 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI ; EI |
| 关键词 | stars: mass-loss supernovae: general ultraviolet: stars |
| 摘要 | The properties of H-rich, type II-plateau supernova (SN II-P) progenitors remain uncertain, and this is primarily due to the complexities associated with red supergiant (RSG) mass loss. Recent studies have suggested that the interaction of the ejecta with a standard RSG wind should produce unambiguous signatures in the optical (e.g., a broad, boxy H alpha profile) and in the UV (especially Ly alpha and MgII lambda lambda 2795, 2802) a few years following the explosion. Such features are expected to be generic in all SNe II-P and can be utilized to constrain RSG winds. Here, we investigate the possibility of detecting late-time (0.3-10 years since explosion) SNe II-P in the NUV with the China Space Station Telescope (CSST). Convolving the existing model spectra of ejecta-wind interactions in SNe II-P with the transmission functions of the CSST, we calculated the associated multiband light curves, in particular, the NUV (255 nm-317 nm) band, as well as the NUV-r color. We find that the CSST will be able to detect the NUV radiation associated with ejecta-wind interaction for hundreds SNe II-P out to a few hundred Mpc over its ten-year main sky survey. The CSST will therefore provide a sizable sample of SNe II-P with the NUV signatures of ejecta-wind interaction. This will be helpful for understanding the mass loss history of SN II-P progenitors and their origins. |
| 资助项目 | National Natural Science Foundation of China (NSFC)[12125303]; National Natural Science Foundation of China (NSFC)[12288102]; National Natural Science Foundation of China (NSFC)[12090040/1]; National Natural Science Foundation of China (NSFC)[11873016]; 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[202201BC070003]; Yunnan Fundamental Research Projects[202001AW070007]; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202305AB350003]; China Manned Space Project[CMS-CSST-2021-A10] |
| 项目资助者 | National Natural Science Foundation of China (NSFC)[12125303, 12288102, 12090040/1, 11873016] ; 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[202201BC070003, 202001AW070007] ; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202305AB350003] ; China Manned Space Project[CMS-CSST-2021-A10] |
| 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 | EDP SCIENCES S A |
| 出版地 | 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE |
| ISSN | 0004-6361 |
| URL | 查看原文 |
| WOS记录号 | WOS:001366206400002 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | CORE-COLLAPSE SUPERNOVAE ; LIGHT-CURVES ; SN 2010JL ; CIRCUMSTELLAR INTERACTION ; CHEMICAL ENRICHMENT ; INITIAL MASSES ; EXPLOSION ; PROGENITORS ; EVOLUTION ; NUCLEOSYNTHESIS |
| EI入藏号 | 20244117156877 |
| EI主题词 | Supernovae |
| EI分类号 | 1302.1.2 - 214.1.1 - 443.1 Atmospheric Properties - 741.3 Optical Devices and Systems |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/27639 |
| 专题 | 双星与变星研究组 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, P.R. China; 2.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650216, P.R. China; 3.University of Chinese Academy of Sciences, Beijing 100049, P.R. China; 4.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, P.R. China; 5.Institut d’Astrophysique de Paris, CNRS-Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France |
| 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,Dessart, Luc,Chen XF,et al. Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars[J]. ASTRONOMY & ASTROPHYSICS,2024,689. |
| APA | 罗竞霄,Dessart, Luc,陈雪飞,&柳正伟.(2024).Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars.ASTRONOMY & ASTROPHYSICS,689. |
| MLA | 罗竞霄,et al."Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars".ASTRONOMY & ASTROPHYSICS 689(2024). |
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