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arXiv 2103.12431astro-ph.GA
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TMC-1,无星核心硫磺工厂:NCS、HCCS、H2CCS、H2CCCS和C4S的发现和C5S的检测

TMC-1, the starless core sulfur factory: Discovery of NCS, HCCS, H2CCS, H2CCCS, and C4S and detection of C5S

J. Cernicharo, C. Cabezas, M. Agundez, B. Tercero, J. R. Pardo, N. Marcelino, J. D. Gallego, F. Tercero, J. A. Lopez-Perez, P. de Vicente

摘要:

我们首次在太空中探测到含硫物质NCS、HCCS、H2 CCS、H2 CCCS和C4 S。通过观察每个物种的几条线,发现这些分子朝向TMC-1。我们还报告检测C5 S的第一次在冷云通过观察五条线在31-50 GHz的范围。导出的柱密度为N(NCS)=(7.8 +/- 0.6)e11 cm-2,N(HCCS)=(6.8 +/- 0.6)e11 cm-2,N(H2CCS)=(7.8 +/- 0.8)e11 cm-2,N(H2CCCS)=(3.7 +/- 0.4)e11 cm-2,N(C4S)=(3.8 +/- 0.4)e10 cm-2,N(C5S)=(5.0 +/- 1.0)e10 cm-2。观测到的C3 S和C4 S之间的丰度比为340,也就是说,比CCS和C3 S的相应值大约大100倍。观测结果进行了比较与国家的最先进的化学模型,这是只有部分成功地再现所观察到的丰度。这些发现突出表明,需要改进处理含硫物种的化学网络。

英文摘要:

We report the detection of the sulfur-bearing species NCS, HCCS, H2CCS, H2CCCS, and C4S for the first time in space. These molecules were found towards TMC-1 through the observation of several lines for each species. We also report the detection of C5S for the first time in a cold cloud through the observation of five lines in the 31-50 GHz range. The derived column densities are N(NCS) = (7.8 +/- 0.6)e11 cm-2, N(HCCS) = (6.8 +/- 0.6)e11 cm-2, N(H2CCS) = (7.8 +/- 0.8)e11 cm-2, N(H2CCCS) = (3.7 +/- 0.4)e11 cm-2, N(C4S) = (3.8 +/- 0.4)e10 cm-2, and N(C5S) = (5.0 +/- 1.0)e10 cm-2. The observed abundance ratio between C3S and C4S is 340, that is to say a factor of approximately one hundred larger than the corresponding value for CCS and C3S. The observational results are compared with a state-of-the-art chemical model, which is only partially successful in reproducing the observed abundances. These detections underline the need to improve chemical networks dealing with S-bearing species.

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