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--- molecules:ism:hcns [2024/02/01 13:55] – [Thiocyanic acid] mueller
+++ molecules:ism:hcns [2024/04/17 12:50] (current) – [Isothiocyanic acid] mueller
@@ Line 26: / Line 26: @@
 //Astron. Astrophys.// **575**, (2015), Art. No. A84.\\
 The molecules were identified in the course of a line survey of the circumstellar envelope of this O-rich AGB star, aka QX Pup, with the IRAM 30 m dish at 3 to 1 mm.\\
+\\
+M. Sanz-Novo, V. M. Rivilla, I. Jiménez-Serra, J. Martín-Pintado, L. Colzi, S. Zeng, A. Megías, Á. López-Gallifa, A. Martínez-Henares, S. Massalkhi, B. Tercero, P. de Vicente, D. San Andrés, S. Martín, and M. A. Requena-Torres\\
+announced the\\
+**[[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).\\
+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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-Contributor(s): H. S. P. Müller; 09, 2009; 02, 2024
+Contributor(s): H. S. P. Müller; 09, 2009; 02, 2024; 04, 2024
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