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Chemistry of NH2OH and its related species in the ISM
Zhao, Guoming1,2; He, Mingwei1; Quan, Donghui2; Li, Dalei3; Yang, Xue1; Chang, Qiang4; Ma, Ming-Shuo5; Qu, Minglei1
2023-05-23
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume523Issue:1Pages:1-22
Contribution Rank3
AbstractHydroxylamine (NH2OH) is a key precursor of both the formation of amino acids and the concurrent synthesis of pyrimidine and purine nucleosides. Recently, NH2OH was detected towards the quiescent molecular cloud G+0.693-0.027, which is located in the Galactic Centre. In this study, we construct the chemical network for NH2OH and its related species via quantum chemical calculations, and simulate their chemistry using the astrochemical code Nautilus in isothermal models and shock models. According to the disagreement distance formula and molecular abundance ratios, we acquire the best-fitting isothermal model T18 and the best-fitting C-shock model S2, respectively. Of these two models, S2 is more suitable for G+0.693-0.027 due to its reproduction of abundances of all considered molecules. From the model, we found that NH2OH and CH3NH2 are mainly formed on grain surfaces, while HNCN and CH2NH, which are the post-shock tracers, are produced by both gas-phase and grain-surface reactions. Our chemical modelling also agrees with the observed abundances or upper limits of NH2OH and its related species towards IRAS 16293-2422 B and Sgr B2(N). Moreover, we predict that NH2OH and the undiscovered species H2NO and HNOH are of high abundance, thus are detectable in cold clouds and pre-stellar cores, and in G+0.693-0.027, respectively.
Keywordastrochemistry shock waves ISM: abundances ISM: molecules
DOI10.1093/mnras/stad1379
Indexed BySCI
Language英语
WOS KeywordGAS-GRAIN CHEMISTRY ; COMPLEX ORGANIC-MOLECULES ; DENSE INTERSTELLAR CLOUDS ; STAR-FORMING REGIONS ; BASIS-SETS ; THERMOCHEMICAL KINETICS ; CHEMICAL-COMPOSITION ; CORRELATION-ENERGY ; SAGITTARIUS B2 ; DUST GRAINS
Funding ProjectScience and Technology Research Project of Jilin Provincial Education Department[JJKH20220235KJ] ; Science and Technology Research Project of Jilin Provincial Education Department[JJKH20220232KJ] ; National Natural Science Foundation of China[11973075] ; National Natural Science Foundation of China[11904126] ; National Natural Science Foundation of China[12173075] ; National Natural Science Foundation of China[12173023] ; Youth Innovation Promotion Association CAS ; Tianshan Innovation Team Plan of Xinjiang Uygur Autonomous Region[2022D14020]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000996062900001
PublisherOXFORD UNIV PRESS
Funding OrganizationScience and Technology Research Project of Jilin Provincial Education Department ; National Natural Science Foundation of China ; Youth Innovation Promotion Association CAS ; Tianshan Innovation Team Plan of Xinjiang Uygur Autonomous Region
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Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5259
Collection中国科学院新疆天文台
Corresponding AuthorZhao, Guoming; Quan, Donghui; Yang, Xue
Affiliation1.Jilin Inst Chem Technol, Sch Sci, Jilin 132022, Jilin, Peoples R China
2.Zhejiang Lab, Res Ctr Intelligent Comp Platforms, Hangzhou 311100, Zhejiang, Peoples R China
3.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
4.Shandong Univ Technol, Sch Phys & Optoeletron Engn, Zibo 255000, Shandong, Peoples R China
5.Jilin Inst Chem Technol, Ctr Anal & Measurement, Jilin 132022, Jilin, Peoples R China
Recommended Citation
GB/T 7714
Zhao, Guoming,He, Mingwei,Quan, Donghui,et al. Chemistry of NH2OH and its related species in the ISM[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,523(1):1-22.
APA Zhao, Guoming.,He, Mingwei.,Quan, Donghui.,Li, Dalei.,Yang, Xue.,...&Qu, Minglei.(2023).Chemistry of NH2OH and its related species in the ISM.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,523(1),1-22.
MLA Zhao, Guoming,et al."Chemistry of NH2OH and its related species in the ISM".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 523.1(2023):1-22.
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