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Spatial distributions of 13CO and CS in a carbon-rich AGB star IRC+10216
Tuo, Juan1,2; Yang, Xiaofeng1,3; Sun, Jixian4,5
2024-06-26
Source PublicationFRONTIERS IN ASTRONOMY AND SPACE SCIENCES
ISSN2296-987X
Volume11Pages:1431250
Contribution Rank1
AbstractIRC+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.
Keywordasymptotic giant branch star circumstellar envelope IRC+10216 molecular line (CO)-C-13 CS
DOI10.3389/fspas.2024.1434219
Indexed BySCI
Language英语
WOS KeywordCIRCUMSTELLAR ENVELOPE ; LINE SURVEY ; IRC +10216 ; SIS ; EMISSION ; SULFUR
Funding ProjectNational SKA Program of China[2022SKA0110203] ; XY's CAS Pioneer Hundred Talents Program
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001268488900001
PublisherFRONTIERS MEDIA SA
Funding OrganizationNational SKA Program of China ; XY's CAS Pioneer Hundred Talents Program
Citation statistics
Document Type期刊论文
Identifierhttp://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 AuthorYang, Xiaofeng
Affiliation1.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 AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang 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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