molecules:ism:menh2

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molecules:ism:menh2 [2023/03/06 13:52] – muellermolecules: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\\ 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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 carried out a study on\\ carried out a study on\\
 **[[https://doi.org/10.1093/mnras/sty1174|Complex Organic Molecules in the Galactic Centre: the N-bearing Family]]**\\ **[[https://doi.org/10.1093/mnras/sty1174|Complex Organic Molecules in the Galactic Centre: the N-bearing Family]]**\\
 +//Mon. Not. R. Astron. Soc.// **478**, 2962–2975 (2018).\\
 They performed an unbiased molecular line survey of the quiescent molecular cloud G+0.693−0.03 using the GBT 100 m dish (12.7–15.5 GHz and sections of 18–27 GHz) and the IRAM 30 m dish (80–116, 128–176, and 240–272 GHz). The detected five lines of methylamine.\\ They performed an unbiased molecular line survey of the quiescent molecular cloud G+0.693−0.03 using the GBT 100 m dish (12.7–15.5 GHz and sections of 18–27 GHz) and the IRAM 30 m dish (80–116, 128–176, and 240–272 GHz). The detected five lines of methylamine.\\
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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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