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Spatial distributions of 13CO and CS in a carbon-rich AGB star IRC+10216 | |
Tuo, Juan1,2![]() ![]() | |
2024-06-26 | |
Source Publication | FRONTIERS IN ASTRONOMY AND SPACE SCIENCES
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ISSN | 2296-987X |
Volume | 11Pages:1431250 |
Contribution Rank | 1 |
Abstract | IRC+10216 is the typical carbon-rich asymptotic giant branch star, and more than 100 species have been observed in its circumstellar envelope so far. The use of interferometric arrays to map molecular emission in this source has been widely reported, but to study the angular extent of molecular emission, single-dish mapping must be employed. We report here the mapping of the (CO)-C-13 J = 1-0 and CS J = 2-1 lines towards IRC+10216 using the 13.7 m mm-wave radio telescope at Purple Mountain Observatory. As far as we know, these maps are the largest published (CO)-C-13 J = 2-1 and CS J = 2-1 images to date. Both molecules have roughly spherically symmetric distribution, with (CO)-C-13 having an emission radius of over 80 '' and CS extending up to similar to 50 ''. Assuming that the two molecules are in local thermodynamic equilibrium, the column density and fractional abundance relative to H-2 for (CO)-C-13 and the lower limits for CS are obtained. They are 4.35 x 10(16) cm(-2) and > 4.72 x 10(14) cm(-2), and 5.25 x 10(-5) and > 2.56 x 10(-7) for (CO)-C-13 and CS, respectively. |
Keyword | asymptotic giant branch star circumstellar envelope IRC+10216 molecular line (CO)-C-13 CS |
DOI | 10.3389/fspas.2024.1434219 |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | CIRCUMSTELLAR ENVELOPE ; LINE SURVEY ; IRC +10216 ; SIS ; EMISSION ; SULFUR |
Funding Project | National SKA Program of China[2022SKA0110203] ; XY's CAS Pioneer Hundred Talents Program |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:001268488900001 |
Publisher | FRONTIERS MEDIA SA |
Funding Organization | National SKA Program of China ; XY's CAS Pioneer Hundred Talents Program |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/6843 |
Collection | 射电天文研究室_理论天体物理研究团组 射电天文研究室_天体化学研究团组 |
Corresponding Author | Yang, Xiaofeng |
Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi, Xinjiang, Peoples R China 2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China 3.Xinjiang Key Lab Radio Astrophys, Urumqi, Xinjiang, Peoples R China 4.Chinese Acad Sci, Purple Mt Observ, Nanjing, Peoples R China 5.Chinese Acad Sci, Key Lab Radio Astron, Nanjing, Peoples R China |
First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Recommended Citation GB/T 7714 | Tuo, Juan,Yang, Xiaofeng,Sun, Jixian. Spatial distributions of 13CO and CS in a carbon-rich AGB star IRC+10216[J]. FRONTIERS IN ASTRONOMY AND SPACE SCIENCES,2024,11:1431250. |
APA | Tuo, Juan,Yang, Xiaofeng,&Sun, Jixian.(2024).Spatial distributions of 13CO and CS in a carbon-rich AGB star IRC+10216.FRONTIERS IN ASTRONOMY AND SPACE SCIENCES,11,1431250. |
MLA | Tuo, Juan,et al."Spatial distributions of 13CO and CS in a carbon-rich AGB star IRC+10216".FRONTIERS IN ASTRONOMY AND SPACE SCIENCES 11(2024):1431250. |
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Tuo-2024-Spatial dis(15246KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text |
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