molecules:ism:menh2

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Last revisionBoth sides next revision
molecules:ism:menh2 [2023/03/06 14:37] muellermolecules:ism:menh2 [2023/09/05 14:38] mueller
Line 22: Line 22:
 \\ \\
  
-T. Kamiński, K. M. Menten, R. Tylenda, MHajdukN. A. Patel, and A. Kraus\\+T. Kamiński, K. M. Menten, R. Tylenda, AKarakas, 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.\\
 \\ \\
  
Line 41: Line 42:
 The authors describe the first unambigous detection of methylamine outside of the Galactic center.\\ The authors describe the first unambigous detection of methylamine outside of the Galactic center.\\
 \\ \\
 +
 +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).\\
  
  
 ---- ----
  
-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.
  
 ---- ----
  
  
  • molecules/ism/menh2.txt
  • Last modified: 2023/09/05 14:43
  • by mueller