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星际冰类似物中形成最简单的硫羟酸(HCOSH)─硫羟酸。

Formation of Thioformic Acid (HCOSH)─The Simplest Thioacid─in Interstellar Ice Analogues.

机构信息

Department of Chemistry and W. M. Keck Research Laboratory in Astrochemistry, University of Hawai'i at Manoa, 2545 McCarthy Mall, Honolulu, Hawaii 96822, United States.

Department of Chemistry and Biochemistry, Florida International University, Miami, Florida 33199, United States.

出版信息

J Phys Chem A. 2022 Dec 29;126(51):9699-9708. doi: 10.1021/acs.jpca.2c06860. Epub 2022 Dec 19.

Abstract

Since the observation of the first sulfur-containing molecule, carbon monosulfide (CS), in the interstellar medium (ISM) half a century ago, sulfur-bearing species have attracted great attention from the astrochemistry, astrobiology, and planetary geology communities. Nevertheless, it is still not clear in which forms most of the sulfur resides in molecular clouds, an unsolved problem referred to as "sulfur depletion". Reported herein is the formation of thioformic acid (HCOSH)─the simplest thioacid─in interstellar ice analogues containing carbon monoxide (CO) and hydrogen sulfide (HS) at 5 K. Utilizing single photoionization reflectron time-of-flight mass spectrometry and isotopically labeled molecules, thioformic acid molecules were selectively photoionized in the temperature-programmed desorption phase. These studies unravel a key reaction pathway to thioformic acid, an organic molecule recently detected toward the giant molecular cloud G+0.693-0.027 and the hot core G31.41+0.31, thus shedding light on interstellar sulfur chemistry.

摘要

自半个世纪前首次在星际介质(ISM)中观察到含硫分子一硫化碳(CS)以来,含硫物种引起了天体化学、天体生物学和行星地质学领域的极大关注。然而,在分子云中大多数硫以何种形式存在仍不清楚,这是一个尚未解决的问题,被称为“硫耗竭”。本文报道了在含有一氧化碳(CO)和硫化氢(HS)的星际冰类似物中于 5 K 下形成硫代甲酸(HCOSH)─最简单的硫羧酸─的过程。利用单光致电离反射飞行时间质谱和同位素标记分子,在程序升温脱附相中选择性地光致电离硫代甲酸分子。这些研究揭示了硫代甲酸形成的关键反应途径,硫代甲酸是一种最近在大质量分子云 G+0.693-0.027 和热核 G31.41+0.31 中检测到的有机分子,从而为星际硫化学提供了新的认识。

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