Laboratory Rotational Spectroscopy Leads to the First Interstellar Detection of Singly Deuterated Methyl Mercaptan (CH2DSH)

Hayley A. Bunn, Silvia Spezzano, Laurent H. Coudert, Jean-Claude Guillemin, Yuxin Lin, Christian P. Endres, Brant Billinghurst, Olivier Pirali, Jes Jørgensen, Valerio Lattanzi and Paola Caselli
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Abstract

We report an extensive rotational spectroscopic analysis of singly deuterated methyl mercaptan (CH2DSH) using both millimeter and far-infrared synchrotron spectra to achieve a global torsional analysis of the three lowest torsional substates (e0, e1, and o1) of this nonrigid species. A fit including 3419 millimeter-wave transitions along with 43 infrared torsional subband centers was performed with rms deviations of 0.233 MHz and 0.270 cm−1, respectively, resulting in 68 fit parameters. A spectroscopic catalog built from this analysis for a temperature of 125 K has led to the first interstellar detection of CH2DSH toward the solar-like protostar IRAS 16293-2422 B. We report the identification of 46 transitions, including eight relatively unblended lines, resulting in a derived column density of (3.0 ± 0.3) × 1014 cm−2. The column density ratio for HDCS/CH2DSH compared to HDCO/CH2DOH suggests a difference in the interstellar chemistry between the sulfur and oxygen complex organics, in particular a different link between H2CO and CH3OH and between H2CS and CH3SH. This is the first interstellar detection of a deuterated sulfur-bearing complex organic molecule and therefore an important step toward understanding the chemical origin of sulfur-based prebiotics.
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实验室旋转光谱导致首次星际探测到单氘化甲基硫醇(CH2DSH)
我们报道了一个广泛的旋转光谱分析的单氘化甲基硫醇(CH2DSH)使用毫米和远红外同步辐射光谱实现了三个最低扭转亚态(e0, e1和o1)的非刚性物质的整体扭转分析。对3419个毫米波跃迁和43个红外扭转子带中心进行了拟合,其rms偏差分别为0.233 MHz和0.270 cm−1,得到了68个拟合参数。根据这一分析,在125 K的温度下建立了一个光谱目录,导致CH2DSH首次在星际间探测到类似太阳的原恒星IRAS 16293-2422 b。我们报告了46个转变的识别,包括8个相对未混合的谱线,得出的柱密度为(3.0±0.3)× 1014 cm−2。HDCS/CH2DSH的柱密度比与HDCO/CH2DOH的柱密度比表明了硫氧复合有机物之间的星际化学差异,特别是H2CO和CH3OH之间以及H2CS和CH3SH之间的不同联系。这是第一次星际探测到氘化含硫复杂有机分子,因此是了解含硫益生元化学起源的重要一步。
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