首次发现星际介质中新的含硫醇 (-SH) 分子并建立化学模型:二硫代甲酸

IF 2.9 3区 化学 Q2 CHEMISTRY, MULTIDISCIPLINARY
Arijit Manna*,  and , Sabyasachi Pal, 
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引用次数: 0

摘要

由于- SH在氨基酸(R-CH (NH2) -COOH)的聚合中起着重要作用,因此对含有巯基(- SH)的复杂有机分子的研究在星际介质中是必不可少的。一些量子化学研究表明,在热分子核和热粒子的高密度和温暖的内部区域,有很高的机会探测到二硫代甲酸(HC(S)SH)的发射谱线。因此,我们尝试使用阿塔卡马大毫米/亚毫米阵列(ALMA)波段7搜索HC(S)SH对高密度热corino物体NGC 1333 IRAS 4A的发射线。我们首次探测到二硫代甲酸反式构象(t-HC(S)SH)对NGC 1333 IRAS 4A2的旋转发射谱线。t-HC(S)SH对NGC 1333 IRAS 4A2的柱密度和激发温度分别为(2.63±0.32)× 1015 cm-2和255±32 K。t-HC(S)SH相对于H2的丰度为(2.53±0.68)× 10-9。t-HC(S)SH与t-HCOOH对NGC 1333 IRAS 4A2的柱密度比为0.36±0.02。为了了解HC(S)SH可能的形成途径,我们使用气粒化学代码UCLCHEM计算了HC(S)SH的两相预热化学模型丰度。经过化学建模,我们认为在NGC 1333 IRAS 4A2中,HC(S)SH是通过晶粒表面的CSSH和H之间的自由基-自由基反应形成的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

First Identification and Chemical Modeling of New Thiol (−SH) Bearing Molecule in the Interstellar Medium: Dithioformic Acid

First Identification and Chemical Modeling of New Thiol (−SH) Bearing Molecule in the Interstellar Medium: Dithioformic Acid

The study of complex organic molecules containing thiol (−SH) groups is essential in interstellar media because −SH plays an important role in the polymerization of amino acids (R–CH(NH2)–COOH). Some quantum chemical studies have shown that there is a high chance of detecting the emission lines of dithioformic acid (HC(S)SH) in the highly dense and warm-inner regions of hot molecular cores and hot corinos. Therefore, we attempted to search for the emission lines of HC(S)SH toward the highly dense hot corino object NGC 1333 IRAS 4A using the Atacama Large Millimeter/Submillimeter Array (ALMA) band 7. We present the first detection of the rotational emission lines of the trans-conformer of dithioformic acid (t-HC(S)SH) toward the NGC 1333 IRAS 4A2. The column density and excitation temperature of the t-HC(S)SH toward NGC 1333 IRAS 4A2 are (2.63 ± 0.32) × 1015 cm–2 and 255 ± 32 K, respectively. The fractional abundance of t-HC(S)SH with respect to H2 is (2.53 ± 0.68) × 10–9. The column density ratio of t-HC(S)SH and t-HCOOH toward NGC 1333 IRAS 4A2 is 0.36 ± 0.02. To understand the possible formation pathways of HC(S)SH, we computed a two-phase warm-up chemical model abundance of HC(S)SH using the gas-grain chemical code UCLCHEM. After chemical modeling, we claim that HC(S)SH is formed in NGC 1333 IRAS 4A2 via barrierless radical–radical reactions between CSSH and H on the grain surfaces.

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来源期刊
ACS Earth and Space Chemistry
ACS Earth and Space Chemistry Earth and Planetary Sciences-Geochemistry and Petrology
CiteScore
5.30
自引率
11.80%
发文量
249
期刊介绍: The scope of ACS Earth and Space Chemistry includes the application of analytical, experimental and theoretical chemistry to investigate research questions relevant to the Earth and Space. The journal encompasses the highly interdisciplinary nature of research in this area, while emphasizing chemistry and chemical research tools as the unifying theme. The journal publishes broadly in the domains of high- and low-temperature geochemistry, atmospheric chemistry, marine chemistry, planetary chemistry, astrochemistry, and analytical geochemistry. ACS Earth and Space Chemistry publishes Articles, Letters, Reviews, and Features to provide flexible formats to readily communicate all aspects of research in these fields.
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