This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision | |
| molecules:ism:hc_ns [2024/08/14 16:16] – mueller | molecules:ism:hc_ns [2024/12/10 16:07] (current) – mueller |
|---|
| **[[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 ethenthionyl radical, HCCS, was identified through 2 <sup>1</sup>H hyperfine components of the <sup>2</sup>Π<sub>3/2</sub> //J// = 7/2 − 5/2 transition near 41.1 GHz 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 column density is slightly lower than that of H<sub>2</sub>CCS and about a factor of ten lower than that of HCS.\\ | The ethynylsulfanyl radical, HCCS, was identified through 2 <sup>1</sup>H hyperfine components of the <sup>2</sup>Π<sub>3/2</sub> //J// = 7/2 − 5/2 transition near 41.1 GHz 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 column density is slightly lower than that of H<sub>2</sub>CCS and about a factor of ten lower than that of HCS.\\ |
| \\ | \\ |
| |