中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A 3 mm molecular line survey toward the C-star envelope CIT 6

文献类型:期刊论文

作者Yang, Kuilu5; Zhang, Yong3,4,5; Qiu, Jianjie2,3,5; Ao, Yina5; Li, Xiaohu1,4
刊名PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
出版日期2023-07-18
页码21
ISSN号0004-6264
关键词circumstellar matter ISM: molecules radio lines: stars stars: AGB and post-AGB
DOI10.1093/pasj/psad043
通讯作者Zhang, Yong(zhangyong5@mail.sysu.edu.cn)
英文摘要We present an unbiased molecular line survey toward the carbon-rich circumstellar envelope CIT 6 carried out between 90 and 116 GHz with the Arizona Radio Observatory 12 m telescope. A total of 42 lines assigned to 10 molecular species and four isotopologues are detected. Despite the absence of any newly identified circumstellar molecules, several transitions are freshly reported for this object. This work is a complement to our previous line survey toward CIT 6 in the frequency ranges of 36-49 GHz and 131-268 GHz. Based on the measurements and in combination with previously published data, we perform a rotation-diagram analysis to determine the column densities, excitation temperatures, and fractional abundances of the molecules. The excitation temperature varies along the radius. The abundance pattern of CIT 6 is broadly consistent with that of the prototype C-star IRC +10216 at the specified detection sensitivity, indicating that the molecular richness in IRC +10216 cannot be attributed to an interpretation of unusual chemistry. Nevertheless, subtle distinctions between the two C-stars are found. The higher abundance of carbon-chain molecules and lower C-12/C-13 ratio in CIT 6 compared to IRC +10216 imply that the former is more massive or in a more evolved phase than the latter.
WOS关键词MASS-LOSS RATES ; RICH CIRCUMSTELLAR ENVELOPES ; EVOLVED STARS ; CARBON-MONOXIDE ; RED GIANTS ; PROTOPLANETARY DISK ; PLANETARY-NEBULAE ; COLOGNE DATABASE ; O-RICH ; EMISSION
资助项目National Science Foundation of China(NSFC)[11973099] ; National Science Foundation of China(NSFC)[12003080] ; China Manned Space Project[CMS-CSST-2021-A09] ; China Manned Space Project[CMS-CSST-2021-A10] ; Guang-dong Basic and Applied Basic Research Foundation[2019A1515110588] ; Fundamental Research Funds for the Central Universities[22qntd3101]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:001033392000001
资助机构National Science Foundation of China(NSFC) ; China Manned Space Project ; Guang-dong Basic and Applied Basic Research Foundation ; Fundamental Research Funds for the Central Universities
源URL[http://ir.xao.ac.cn/handle/45760611-7/5322]  
专题研究单元未命名
通讯作者Zhang, Yong
作者单位1.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China
2.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China
3.Sun Yat Sen Univ, CSST Sci Ctr Guangdong Hongkong Macau Greater Bay, Zhuhai 519000, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
5.Sun Yat Sen Univ, Sch Phys & Astron, 2 Da Xue Rd, Zhuhai 519000, Guangdong, Peoples R China
推荐引用方式
GB/T 7714
Yang, Kuilu,Zhang, Yong,Qiu, Jianjie,et al. A 3 mm molecular line survey toward the C-star envelope CIT 6[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2023:21.
APA Yang, Kuilu,Zhang, Yong,Qiu, Jianjie,Ao, Yina,&Li, Xiaohu.(2023).A 3 mm molecular line survey toward the C-star envelope CIT 6.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,21.
MLA Yang, Kuilu,et al."A 3 mm molecular line survey toward the C-star envelope CIT 6".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN (2023):21.

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