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--- molecules:ism:menh2 [2023/03/06 14:37] – mueller
+++ molecules:ism:menh2 [2023/09/05 14:43] (current) – mueller
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-T. Kamiński, K. M. Menten, R. Tylenda, M. Hajduk, N. A. Patel, and A. Kraus\\
+T. Kamiński, K. M. Menten, R. Tylenda, A. Karakas, A. Belloche, and N. A. Patel\\
 investigated the\\
-**[[https://doi.org/10.1038/nature14257|Spectral scan of Orion A and IRC+10216 from 72 to 91 GHz]]**\\
+**[[https://doi.org/10.1051/0004-6361/201731287|Organic Molecules, Ions, and Rare Isotopologues in the Remnant of the Stellar-merger Candidate, CK Vulpeculae (Nova 1670)]]**\\
-//Nature// **520**, 322–324 (2015).\\
+//Astron. Astrophys.// **607**, Art. No. A78 (2017).\\
+Methylamine was identified through several transitions covered by the IRAM 30 m and APEX 12 m telescopes.\\
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+P. Gyawali, R. A. Motiyenko, A. Belloche, I. Kleiner, V. V. Ilyushin, E. A. Alekseev, I. Gulaczyk and M. Kreglewski\\
+described the\\
+**[[https://doi.org/10.1051/0004-6361/202346518|Rotational Spectrum and Interstellar Detection of the First Torsionally Excited State of Methylamine]]**\\
+//Astron. Astrophys.// **677**, Art. No. A65 (2023).\\
+Five lines in //v//<sub>t</sub> = 1 were reported as blended or only slightly blended in addition to ten in //v//<sub>t</sub> = 0. The observational data are from the ReMoCA survey of Sagittarius B2(N) carried out with ALMA at 3 mm.\\
+\\
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-Contributor(s): H. S. P. Müller; 03, 2016; 06, 2019; 08, 2020; 03, 2023.
+Contributor(s): H. S. P. Müller; 03, 2016; 06, 2019; 08, 2020; 03, 2023; 09, 2023.
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