XAO OpenIR  > 射电天文研究室  > 天体化学研究团组
Correlations of methyl formate (CH3OCHO), dimethyl ether (CH3OCH3), and ketene (H2CCO) in high-mass star-forming regions
Li, Chuanshou1; Qin, Sheng-Li1; Liu, Tie2; Liu, Sheng-Yuan3; Tang, Mengyao4; Liu, Hong-Li1; Chen, Li1; Li, Xiaohu5; Xu, Fengwei6,7; Zhang, Tianwei8,9; Liu, Meizhu1; Shi, Hongqiong1; Wu, Yuefang7
2024-08-21
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume533Issue:2Pages:1583-1617
Contribution Rank5
AbstractWe present high-spatial resolution (0.7-1.0 arcsec) submillimeter observations of continuum and molecular lines of CH3OCHO, CH3OCH3, and H2CCO toward 11 high-mass star-forming regions using the Atacama large millimetre/submillimetre array (ALMA). A total of 19 separate cores from nine high-mass star-forming regions are found to be line-rich, including high-, intermediate-, and low-mass line-rich cores. The three molecules are detected in these line-rich cores. We map the emission of CH3OCHO, CH3OCH3, and H2CCO in nine high-mass star-forming regions. The spatial distribution of the three molecules is very similar and concentrated in the areas of intense continuum emission. We also calculate the rotation temperatures, column densities, and abundances of CH3OCHO, CH3OCH3, and H2CCO under the local thermodynamic equilibrium assumption. The abundances relative to H-2 and CH3OH, and line widths of the three molecules are significantly correlated. The abundances relative to H-2, temperatures, and line widths of the three molecules tend to be higher in cores with higher mass and outflows detected. The possible chemical links of the three molecules are discussed.
KeywordAstrochemistry ISM: molecules star: formation
DOI10.1093/mnras/stae1934
Indexed BySCI
Language英语
WOS KeywordCOMPLEX ORGANIC-MOLECULES ; ALMA 3-MILLIMETER OBSERVATIONS ; GAS-GRAIN CHEMISTRY ; HOT CORE ; GALACTIC-CENTER ; SPECTRAL SURVEY ; LINE SURVEY ; MILLIMETER ; PHASE ; ATOMS
Funding ProjectALMA[2022YFA1603101] ; National Key RAMP ; D Program of China[12203011] ; NSFC ; Xinjiang Uygur Autonomous Region of China[202101BA070001-261] ; Yunnan provincial Department of Science and Technology
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001299560400015
PublisherOXFORD UNIV PRESS
Funding OrganizationALMA ; National Key RAMP ; D Program of China ; NSFC ; Xinjiang Uygur Autonomous Region of China ; Yunnan provincial Department of Science and Technology
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6957
Collection射电天文研究室_天体化学研究团组
Corresponding AuthorLi, Chuanshou
Affiliation1.Yunnan Univ, Sch Phys & Astron, Kunming 650091, Peoples R China
2.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
3.Acad Sinica, Inst Astron & Astrophys, 11F AS NTU Astron Math Bldg,1,Roosevelt Rd,Sect 4, Taipei 10617, Taiwan
4.Chuxiong Normal Univ, Inst Astrophys, Sch Phys & Elect Sci, Chuxiong 675000, Peoples R China
5.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 831399, Peoples R China
6.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
7.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
8.Univ Cologne, Phys Inst 1, Zulpicher Str 77, D-50937 Cologne, Germany
9.Zhejiang Lab, Res Ctr Intelligent Comp Platforms, Hangzhou 311100, Peoples R China
Recommended Citation
GB/T 7714
Li, Chuanshou,Qin, Sheng-Li,Liu, Tie,et al. Correlations of methyl formate (CH3OCHO), dimethyl ether (CH3OCH3), and ketene (H2CCO) in high-mass star-forming regions[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,533(2):1583-1617.
APA Li, Chuanshou.,Qin, Sheng-Li.,Liu, Tie.,Liu, Sheng-Yuan.,Tang, Mengyao.,...&Wu, Yuefang.(2024).Correlations of methyl formate (CH3OCHO), dimethyl ether (CH3OCH3), and ketene (H2CCO) in high-mass star-forming regions.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,533(2),1583-1617.
MLA Li, Chuanshou,et al."Correlations of methyl formate (CH3OCHO), dimethyl ether (CH3OCH3), and ketene (H2CCO) in high-mass star-forming regions".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 533.2(2024):1583-1617.
Files in This Item:
File Name/Size DocType Version Access License
Li-2024-Correlations(10983KB)期刊论文出版稿开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Li, Chuanshou]'s Articles
[Qin, Sheng-Li]'s Articles
[Liu, Tie]'s Articles
Baidu academic
Similar articles in Baidu academic
[Li, Chuanshou]'s Articles
[Qin, Sheng-Li]'s Articles
[Liu, Tie]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Li, Chuanshou]'s Articles
[Qin, Sheng-Li]'s Articles
[Liu, Tie]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: Li-2024-Correlations of methyl formate (CH_sub.pdf
Format: Adobe PDF
This file does not support browsing at this time
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.