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| molecules:ism:hcns [2024/04/17 12:49] – mueller | molecules:ism:hcns [2024/04/17 12:50] (current) – [Isothiocyanic acid] mueller |
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| **[[https://doi.org/10.3847/1538-4357/ad2c01|Interstellar Detection of O-protonated Carbonyl Sulfide, HOCS<sup>+</sup>]]**\\ | **[[https://doi.org/10.3847/1538-4357/ad2c01|Interstellar Detection of O-protonated Carbonyl Sulfide, HOCS<sup>+</sup>]]**\\ |
| //Astrophys. J.// **965**, Art. No. 149 (2024).\\ | //Astrophys. J.// **965**, Art. No. 149 (2024).\\ |
| The results were obtained in the course of a molecular line survey of the Galactic Center molecular cloud G+0.693–0.027 employing the Yebes 40 m and IRAM 30 m radio telecopes. The //K<sub>a</sub>// = 0 lines of HOCS<sup>+</sup> were blended with those of HNC<sup>34</sup>S because of nearly identical values of //B + C//. The transitions cover 34 to 161 GHz with //J"// = 2, 3, 6 − 13 and //K<sub>a</sub>// = 0. The contribution of HNC<sup>34</sup>S could be accounted for accurately through lines of HNCS, OCS, and OC<sup>34</sup>S and turned out to be less than that of HOCS<sup>+</sup>. Several lines are slightly or more severely blended in addition, but this is in most cases also well accounted.\\ | The results were obtained in the course of a molecular line survey of the Galactic Center molecular cloud G+0.693–0.027 employing the Yebes 40 m and IRAM 30 m radio telecopes. The //K<sub>a</sub>// = 0 lines of HOCS<sup>+</sup> were blended with those of HNC<sup>34</sup>S because of nearly identical values of //B + C//. The transitions cover 34 to 161 GHz with //J"// = 2, 3, 6 − 13. The contribution of HNC<sup>34</sup>S could be accounted for accurately through lines of HNCS, OCS, and OC<sup>34</sup>S and turned out to be less than that of HOCS<sup>+</sup>. Several lines are slightly or more severely blended in addition, but this is in most cases also well accounted.\\ |
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