实验室旋转光谱导致首次星际探测到单氘化甲基硫醇(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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摘要

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