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--- molecules:ism:menc [2023/09/26 10:23] – mueller
+++ molecules:ism:menc [2023/09/26 10:35] (current) – mueller
@@ Line 25: / Line 25: @@
 H. Calcutt, M. R. Fiechter, E. R. Willis, H. S. P. Müller, R. T. Garrod, J. K. Jørgensen, S. F. Wampfler, T. L. Bourke, A. Coutens, M. N. Drozdovskaya, N. F. W. Ligterink, and L. E. Kristensen,\\
 reported on\\
-[[https://doi.org/10.1051/0004-6361/201833140|The ALMA-PILS survey: First detection of methyl isocyanide (CH<sub>3</sub>NC) in a solar-type protostar]]\\
+**[[https://doi.org/10.1051/0004-6361/201833140|The ALMA-PILS survey: First detection of methyl isocyanide (CH<sub>3</sub>NC) in a solar-type protostar]]**\\
-//Astron. Astrophys.// **** (2018), in press.\\
+//Astron. Astrophys.// **617** (2018), Art. No. A95.\\
 Several transitions with //J// = 17 – 16 and 18 – 17 and //K// between 0 and 7 were detected near 342 and 362 GHz, respectively toward source B. The molecule was not detected toward source A. The CH<sub>3</sub>CN to CH<sub>3</sub>NC ratio is about 200 toward source B and more than 5000 toward source A.\\
 \\
+J. D. Tennis, C. Xue, D. Talbi, P. B. Changala, M. L. Sita, B. McGuire, and E Herbst\\
+announced the\\
+**[[https://doi.org/10.1093/mnras/stad2398|Detection and Modelling of CH<sub>3</sub>NC in TMC-1]]**\\
+//Mon. Not. R. Astron. Soc.// **525**, 2154–2171 (2023).\\
+The //J// = 1 − 0 transition near 20.105 GHz was detected in the course of the GOTHAM line survey toward TMC-1 with the 100 m GBT. The respective transition of CH<sub>3</sub>CN near 18.40 GHz was also detected and a CH<sub>3</sub>CN : CH<sub>3</sub>NC ratio of ~17 was inferred.\\
+\\