中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A deep search for C2H in the oxygen-rich post-AGB star OH 231.8+4.2

文献类型:期刊论文

作者Yang, Jianchao1,4; Yang, Xiaofeng1,3; Zhu, Cheng1,2
刊名FRONTIERS IN ASTRONOMY AND SPACE SCIENCES
出版日期2024-06-25
卷号11页码:1431250
关键词post-AGB star circumstellar envelopes (CSEs) column density C2H OH 231.8+4.2
ISSN号2296-987X
DOI10.3389/fspas.2024.1431250
产权排序1
英文摘要In carbon-rich environment, C2H emission is seen to be associated with HC3N, but whether it can trace the HC3N molecule in oxygen-rich environment is unknown. Here, we have searched for rotational emission from ethynyl radical (C2H) in the oxygen-rich circumstellar envelope (CSE) of the post-asymptotic giant branch (post-AGB) star OH 231.8+4.2, a renowned galactic proto-planetary nebula (PPN) known to display cyanoacetylene (HC3N) emission. Our observations were conducted using the James Clerk Maxwell Telescope (JCMT), and the total on-source time is 11.9 h. Base on local thermodynamic equilibrium (LTE) excitation analysis, we have calculated the column density and the abundance relative to H-2 for C2H. The calculated column density for C2H is less than 1.4 x 10(13) cm(-2), which corresponds to a fractional abundance, f (C2H), less than 4.5 x 10(-9). This inference suggests that the typical transformation pathway from C2H and C2H2 to HC3N may not play a significant role in O-rich environments. It indicates the presence of alternative, unidentified pathways that contribute to the formation of HC3N in O-rich circumstellar envelopes.
WOS关键词OUTFLOW
资助项目National SKA Program of China[2022SKA0110203] ; Korea Astronomy and Space Science Institute ; National Key R&D Program of China[2017YFA0402700] ; JCMT[E21AZ002] ; JCMT[M23BP059] ; [2024]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001265477400001
出版者FRONTIERS MEDIA SA
资助机构National SKA Program of China ; Korea Astronomy and Space Science Institute ; National Key R&D Program of China ; JCMT
源URL[http://ir.xao.ac.cn/handle/45760611-7/6827]  
专题射电天文研究室_理论天体物理研究团组
通讯作者Yang, Xiaofeng
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Peoples R China
2.Chinese Acad Sci, Inst Chem, Beijing Natl Lab Mol Sci BNLMS, Beijing, Peoples R China
3.Xinjiang Key Lab Radio Astrophys, Urumqi, Peoples R China
4.Univ Chinese Acad Sci, Beijing, Peoples R China
推荐引用方式
GB/T 7714
Yang, Jianchao,Yang, Xiaofeng,Zhu, Cheng. A deep search for C2H in the oxygen-rich post-AGB star OH 231.8+4.2[J]. FRONTIERS IN ASTRONOMY AND SPACE SCIENCES,2024,11:1431250.
APA Yang, Jianchao,Yang, Xiaofeng,&Zhu, Cheng.(2024).A deep search for C2H in the oxygen-rich post-AGB star OH 231.8+4.2.FRONTIERS IN ASTRONOMY AND SPACE SCIENCES,11,1431250.
MLA Yang, Jianchao,et al."A deep search for C2H in the oxygen-rich post-AGB star OH 231.8+4.2".FRONTIERS IN ASTRONOMY AND SPACE SCIENCES 11(2024):1431250.

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