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CHNO异构体的天体化学意义:关于其稳定性和可探测性的计算视角

Astrochemical Significance of CHNO Isomers: A Computational Perspective on Their Stability and Detectability.

作者信息

Noriega Lisset, Gonzalez-Ortiz Luis Armando, Ortíz-Chi Filiberto, Merino Gabriel

机构信息

Departamento de Física Aplicada, Centro de Investigación y de Estudios Avanzados, Unidad Mérida, km 6 Antigua Carretera a Progreso, Apdo. Postal 73, Cordemex 97310 Mérida, Yucatán, Mexico.

Secihti-Departamento de Física Aplicada, Centro de Investigación y de Estudios Avanzados, Unidad Mérida, km 6 Antigua Carretera a Progreso, Apdo. Postal 73, Cordemex 97310 Mérida, Yucatán, Mexico.

出版信息

J Phys Chem A. 2025 May 29;129(21):4715-4723. doi: 10.1021/acs.jpca.5c01086. Epub 2025 May 15.

DOI:10.1021/acs.jpca.5c01086
PMID:40372245
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC12128033/
Abstract

Nitrogen- and oxygen-containing molecules play a key role in interstellar chemistry, particularly as precursors to biologically relevant species such as amino acids. Among the CHNO isomers, 2-aminoethanol is the only one detected in the ISM. This study systematically explores the CHNO chemical space, identifying eight structural isomers, with 1-aminoethanol as the global minimum and methylaminomethanol, 11.5 kcal/mol higher in energy, as a viable higher-energy species. To assess their astrochemical relevance, we conducted a comprehensive conformational analysis and computed rotational constants to guide future spectroscopic searches. These findings provide critical insights into CHNO isomers, identifying new candidates for ISM detection and expanding our understanding of nitrogen- and oxygen-containing organic species in space.

摘要

含氮和氧的分子在星际化学中起着关键作用,尤其是作为诸如氨基酸等与生物相关物种的前体。在CHNO异构体中,2-氨基乙醇是在星际介质中检测到的唯一一种。本研究系统地探索了CHNO化学空间,确定了八种结构异构体,其中1-氨基乙醇能量最低,而甲基氨基甲醇能量比其高11.5千卡/摩尔,是一种可能存在的高能物种。为了评估它们在天体化学中的相关性,我们进行了全面的构象分析并计算了转动常数,以指导未来的光谱搜索。这些发现为CHNO异构体提供了关键见解,确定了星际介质检测的新候选物,并扩展了我们对太空中含氮和氧的有机物种的理解。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/c54264afd019/jp5c01086_0007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/e5d1cea813bc/jp5c01086_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/f85af5aad4d9/jp5c01086_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/8f21d01fcbe3/jp5c01086_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/bf9d528abc99/jp5c01086_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/5798fb7c34b1/jp5c01086_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/4cc4cd3c2407/jp5c01086_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/c54264afd019/jp5c01086_0007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/e5d1cea813bc/jp5c01086_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/f85af5aad4d9/jp5c01086_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/8f21d01fcbe3/jp5c01086_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/bf9d528abc99/jp5c01086_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/5798fb7c34b1/jp5c01086_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/4cc4cd3c2407/jp5c01086_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/38f6/12128033/c54264afd019/jp5c01086_0007.jpg

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本文引用的文献

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CHO Isomers: Insights into Potential Interstellar Species.CHO异构体:对潜在星际物种的见解。
J Phys Chem A. 2024 Nov 21;128(46):9964-9971. doi: 10.1021/acs.jpca.4c04804. Epub 2024 Nov 11.
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In Quest of the Missing CHO Isomers in the Interstellar Medium: A Theoretical Search.探寻星际介质中缺失的CHO异构体:一项理论研究
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Prebiotic Astrochemistry from Astronomical Observations and Laboratory Spectroscopy.基于天文观测与实验室光谱学的益生元天体化学
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Future space experiment platforms for astrobiology and astrochemistry research.用于天体生物学和天体化学研究的未来空间实验平台。
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Recent Advances in N-O Bond Cleavage of Oximes and Hydroxylamines to Construct N-Heterocycle.肟和羟胺中 N-O 键断裂构建 N-杂环的最新进展。
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