Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars
文献类型：期刊论文
| 作者 | Luo JX(罗竞霄)2,3,4,5 ; Dessart, Luc1; Chen XF(陈雪飞)2,4,5; Liu ZW(柳正伟)2,4,5
|
| 刊名 | Astronomy and Astrophysics
 |
| 出版日期 | 2024-09-01 |
| 卷号 | 689 |
| ISSN号 | 0004-6361 |
| DOI | 10.1051/0004-6361/202349123 |
| 产权排序 | 第1完成单位 |
| 文献子类 | Journal article (JA) |
| 英文摘要 | 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 Hα profile) and in the UV (especially Ly α and Mga IIλλ 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. © The Authors 2024. |
| 学科主题 | 天文学 ; 恒星与银河系 |
| URL标识 | 查看原文 |
| 资助项目 | National Natural Science Foundation of China[11873016];National Natural Science Foundation of China[12125303];National Natural Science Foundation of China[12288102] |
| 语种 | 英语 |
| 资助机构 | National Natural Science Foundation of China[11873016, 12125303, 12288102] |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/27639]  |
| 专题 | 云南天文台_双星与变星研究组 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.Institut d'Astrophysique de Paris, CNRS, Sorbonne Université, 98 bis boulevard Arago, Paris, 75014, France 2.International Centre of Supernovae, Yunnan Key Laboratory, Kunming, 650216, China; 3.University of Chinese Academy of Sciences, Beijing, 100049, China; 4.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming, 650216, China; 5.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming, 650216, China; |
| 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 and 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 and 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 and Astrophysics 689(2024). |
入库方式： OAI收割
来源：云南天文台
浏览0
下载0
收藏0
其他版本
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。