Show pageOld revisionsBacklinksBack to top This page is read only. You can view the source, but not change it. Ask your administrator if you think this is wrong. ===== On Cyclopropenethione in the ISM ===== A. J. Remijan, P. B. Changala, C. Xue, E. Q. H. Yuan, M. Duffy, H. N. Scolati, C. N. Shingledecker, T. H. Speak, I. R. Cooke, R. Loomis, A. M. Burkhardt, Z. T. P. Fried, G. Wenzel, A. Lipnicky, M. C. McCarthy, and B. A. McGuire\\ announced\\ **[[https://doi.org/10.3847/1538-4357/adb84c|The Missing Link of Sulfur Chemistry in TMC-1: The Detection of //c//-C<sub>3</sub>H<sub>2</sub>S from the GOTHAM Survey]]**\\ //Astrophys. J.// **982**, Art. No. 191 (2025).\\ The molecule was identified through line-stacking in the course of the GOTHAM survey of TMC-1 carried out with the 100 m GBT dish and covering a large fraction of the 3.9 to 36.4 GHz region. An excitation temperature of ~5 K was derived. The abundance ratio of CH<sub>2</sub>CCS///c//-C<sub>3</sub>H<sub>2</sub>S is about 10 while that of HCCCHS///c//-C<sub>3</sub>H<sub>2</sub>S is about 2.5 (taking into account the differences in assumed source diameters).\\ \\ ---- Contributor(s): H. S. P. Müller; 04, 2025 ---- molecules/ism/cyclopropenonthion.txt Last modified: 2025/04/03 14:30by mueller