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Mapping observations of complex organic molecules around Sagittarius B2 with the ARO 12 m telescope
Li, Juan1,2; Wang, Junzhi1,2; Qiao, Haihua1,2,3; Quan, Donghui4,5; Fang, Min6; Du, Fujun2,7; Li, Fei1,2,8; Shen, Zhiqiang1,2; Li, Shanghuo1,2,8; Li, Di8,9
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2020-02-01
卷号492期号:1页码:556-565
关键词ISM: abundances ISM: clouds ISM: individual (Saggitarius B2) ISM: molecules radio lines: ISM
ISSN号0035-8711
DOI10.1093/mnras/stz3337
英文摘要We have performed high-sensitivity mapping observations of several complex organic molecules around Sagittarius B2 with the ARO 12 m telescope at 3 mm wavelength. Based on their spatial distribution, molecules can be classified as either 'extended', those detected not only in Sgr B2(N) and Sgr B2(M), or 'compact', those only detected toward or near Sgr B2(N) and Sgr B2(M). The 'extended' molecules include glycolaldehyde (CH2OHCHO), methyl formate (CH3OCHO), formic acid (t-HCOOH), ethanol (C2H5OH) and methyl amine (CH3NH2), while the 'compact' molecules include dimethyl ether (CH3OCH3), ethyl cyanide (C2H5CN), and amino acetonitrile (H2NCH2CN). These 'compact' molecules are likely produced under strong UV radiation, while the 'extended' molecules are likely formed at low temperatures, via gas-phase or grain-surface reactions. The spatial distribution of 'warm' CH2OHCHO at 89 GHz differs from the spatial distribution of 'cold' CH2OHCHO observed at 13 GHz. We found evidence for an overabundance of CH2OHCHO compared to that expected from the gas-phase model, which indicates that grain-surface reactions are necessary to explain the origin of CH2OHCHO in Sagittarius B2. Grain-surface reactions are also needed to explain the correlation between the abundances of 'cold' CH2OHCHO and C2H5OH. These results demonstrate the importance of grain-surface chemistry in the production of complex organic molecules.
资助项目National Key R&D Program of China[2017YFA0402604] ; Natural Science Foundation of China[11590780] ; Natural Science Foundation of China[11590782] ; Natural Science Foundation of China[11590784] ; Natural Science Foundation of China[U1731237] ; Natural Science Foundation of China[11773054] ; Natural Science Foundation of China[11725313] ; Natural Science Foundation of China[11690024] ; Natural Science Foundation of China[11903038] ; Special Funding for Advanced Users ; Center for Astronomical Mega-Science ; Chinese Academy of Sciences (CAMS-CAS) ; CAS 'Light of West China' Program
WOS关键词GALACTIC-CENTER ; INTERSTELLAR GLYCOLALDEHYDE ; CHEMISTRY ; SUBMILLIMETER ; REGION ; SCALE ; BAND
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000512329900043
资助机构National Key R&D Program of China ; National Key R&D Program of China ; Natural Science Foundation of China ; Natural Science Foundation of China ; Special Funding for Advanced Users ; Special Funding for Advanced Users ; Center for Astronomical Mega-Science ; Center for Astronomical Mega-Science ; Chinese Academy of Sciences (CAMS-CAS) ; Chinese Academy of Sciences (CAMS-CAS) ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; National Key R&D Program of China ; National Key R&D Program of China ; Natural Science Foundation of China ; Natural Science Foundation of China ; Special Funding for Advanced Users ; Special Funding for Advanced Users ; Center for Astronomical Mega-Science ; Center for Astronomical Mega-Science ; Chinese Academy of Sciences (CAMS-CAS) ; Chinese Academy of Sciences (CAMS-CAS) ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; National Key R&D Program of China ; National Key R&D Program of China ; Natural Science Foundation of China ; Natural Science Foundation of China ; Special Funding for Advanced Users ; Special Funding for Advanced Users ; Center for Astronomical Mega-Science ; Center for Astronomical Mega-Science ; Chinese Academy of Sciences (CAMS-CAS) ; Chinese Academy of Sciences (CAMS-CAS) ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program ; National Key R&D Program of China ; National Key R&D Program of China ; Natural Science Foundation of China ; Natural Science Foundation of China ; Special Funding for Advanced Users ; Special Funding for Advanced Users ; Center for Astronomical Mega-Science ; Center for Astronomical Mega-Science ; Chinese Academy of Sciences (CAMS-CAS) ; Chinese Academy of Sciences (CAMS-CAS) ; CAS 'Light of West China' Program ; CAS 'Light of West China' Program
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/54072]  
专题中国科学院国家天文台
通讯作者Li, Juan
作者单位1.Shanghai Astron Observ, Dept Radio Sci & Technol, 80 Nandan Rd, Shanghai 200030, Peoples R China
2.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China
3.Chinese Acad Sci, Natl Time Serv Ctr, Xian 710600, Shaanxi, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
5.Eastern Kentucky Univ, Dept Chem, Richmond, KY 40475 USA
6.Univ Arizona, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA
7.Chinese Acad Sci, Purple Mt Observ, Nanjing 210034, Peoples R China
8.Univ Chinese Acad Sci, 19A Yuquanlu, Beijing 100049, Peoples R China
9.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing 100101, Peoples R China
10.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China
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GB/T 7714
Li, Juan,Wang, Junzhi,Qiao, Haihua,et al. Mapping observations of complex organic molecules around Sagittarius B2 with the ARO 12 m telescope[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,492(1):556-565.
APA Li, Juan.,Wang, Junzhi.,Qiao, Haihua.,Quan, Donghui.,Fang, Min.,...&Zhang, Jiangshui.(2020).Mapping observations of complex organic molecules around Sagittarius B2 with the ARO 12 m telescope.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,492(1),556-565.
MLA Li, Juan,et al."Mapping observations of complex organic molecules around Sagittarius B2 with the ARO 12 m telescope".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 492.1(2020):556-565.
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