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| molecules:ism:h2c_ns [2022/11/17 12:57] – mueller | molecules:ism:h2c_ns [2022/11/17 12:58] (current) – mueller |
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| **[[https://doi.org/10.1051/0004-6361/202140642|TMC-1, the starless core sulfur factory: Discovery of NCS, HCCS, H<sub>2</sub>CCS, H<sub>2</sub>CCCS, and C<sub>4</sub>S and detection of C<sub>5</sub>S]]**\\ | **[[https://doi.org/10.1051/0004-6361/202140642|TMC-1, the starless core sulfur factory: Discovery of NCS, HCCS, H<sub>2</sub>CCS, H<sub>2</sub>CCCS, and C<sub>4</sub>S and detection of C<sub>5</sub>S]]**\\ |
| //Astron. Astrophys.// **648**, Art. No. L3 (2021).\\ | //Astron. Astrophys.// **648**, Art. No. L3 (2021).\\ |
| The ethenthione, H<sub>2</sub>C<sub>2</sub>S, and propadienthione, H<sub>2</sub>C<sub>3</sub>S, molecules were identified through 6 and 7 //a//-type transitions, respectively, with //K<sub>a</sub>// = 0 and 1 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 between 31.0 and 50.3 GHz. The column density of H<sub>2</sub>C<sub>2</sub>S is about a factor of 100 lower than that of H<sub>2</sub>CS and about a factor of two higher than that of H<sub>2</sub>C<sub>3</sub>S.\\ | The ethenthione, H<sub>2</sub>C<sub>2</sub>S, and propadienthione, H<sub>2</sub>C<sub>3</sub>S, molecules were identified through 6 and 7 //a//-type transitions, respectively, with //K<sub>a</sub>// = 0 and 1 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 between 32.8 and 49.2 GHz. The column density of H<sub>2</sub>C<sub>2</sub>S is about a factor of 100 lower than that of H<sub>2</sub>CS and about a factor of two higher than that of H<sub>2</sub>C<sub>3</sub>S.\\ |
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