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| molecules:ism:c-c6h6s [2026/04/08 11:03] – mueller | molecules:ism:c-c6h6s [2026/04/08 11:08] (current) – mueller |
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| **[[https://doi.org/10.1038/s41550-025-02749-7|A Detection of Sulfur-Bearing Cyclic Hydrocarbons in Space]]**\\ | **[[https://doi.org/10.1038/s41550-025-02749-7|A Detection of Sulfur-Bearing Cyclic Hydrocarbons in Space]]**\\ |
| //Nat. Astron.// **10**, 401 (2026).\\ | //Nat. Astron.// **10**, 401 (2026).\\ |
| The molecule was detected in the course of a molecular line survey of the Galactic Center molecular cloud G+0.693–0.027 employing the Yebes 40 m telecope. The //a//-type transitions cover 31 to 49 GHz with 10 ≤ //J// ≤ 19 and //K<sub>a</sub>// ≤ 7. Some lines are unblended, slightly blended, or the peak of the line is at most slightly blended. Some further lines are blended more substantially. The glycolaldehyde/glycolamide ratio is ∼15, while the ethanol/ethanolamine ratio is ∼40.\\ | 2,5-Cyclohexadienthione was detected in the course of a molecular line survey of the Galactic Center molecular cloud G+0.693–0.027 employing the Yebes 40 m telecope. The //a//-type transitions cover 31 to 49 GHz with 10 ≤ //J// ≤ 19 and //K<sub>a</sub>// ≤ 7. Some lines are unblended, slightly blended, or the peak of the line is at most slightly blended. //T//<sub>rot</sub> ≈ 12.5 K was derived from a rotation diagram. 2,4-Cyclohexadienthione was not detected, its abundance is at least a factor of 2 lower than 2,5-cyclohexadienthione.\\ |
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