molecules:ism:hc3s

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molecules:ism:hc3s [2021/02/26 16:13] muellermolecules:ism:hc3s [2021/02/26 16:14] (current) mueller
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 **[[https://doi.org/10.1051/0004-6361/202040013|Space and laboratory discovery of HC<sub>3</sub>S<sup>+</sup>]]**\\ **[[https://doi.org/10.1051/0004-6361/202040013|Space and laboratory discovery of HC<sub>3</sub>S<sup>+</sup>]]**\\
 //Astron Astrophys.// **646**, Art. No. L3 (2021).\\ //Astron Astrophys.// **646**, Art. No. L3 (2021).\\
-The //J"// = 5 to 8 transitions between 32.8 and 49.2 GHz were detected in the course of a molecular line survey of the prototypical cold dark molecular cloud TMC-1 carried out with the Yebes 40 m radio telescope. The identity was confirmed through laboratory measurements. The C<sub>3</sub>S<sup> to HC<sub>3</sub>S<sup>+</sup> ratio is 65 ± 20, and the HC<sub>3</sub>O<sup>+</sup> to HC<sub>3</sub>S<sup>+</sup> ratio is 1.0 ± 0.5. The C<sub>3</sub>O to C<sub>3</sub>S ratio, in contrast, is ~0.11.+The //J"// = 5 to 8 transitions between 32.8 and 49.2 GHz were detected in the course of a molecular line survey of the prototypical cold dark molecular cloud TMC-1 carried out with the Yebes 40 m radio telescope. The identity was confirmed through laboratory measurements. The C<sub>3</sub>S to HC<sub>3</sub>S<sup>+</sup> ratio is 65 ± 20, and the HC<sub>3</sub>O<sup>+</sup> to HC<sub>3</sub>S<sup>+</sup> ratio is 1.0 ± 0.5. The C<sub>3</sub>O to C<sub>3</sub>S ratio, in contrast, is ~0.11.
  
  
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