molecules:ism:methoxymethanol

Differences

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

Link to this comparison view

Next revisionBoth sides next revision
molecules:ism:methoxymethanol [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:methoxymethanol [2019/07/09 17:04] – added new paper mueller
Line 6: Line 6:
 //Astrophys. J.// **851** L46 (2017).\\ //Astrophys. J.// **851** L46 (2017).\\
 More than two dozen unblended or essentially unblended transitions were detected in several small recordings in Bands 6 and 7 through observations of the high-mass starforming region NGC 6334I-MM1. Assuming an excitation temperature of 200 K, its column density was found to be lower than that of methanol by a factor slightly larger than 30. More than two dozen unblended or essentially unblended transitions were detected in several small recordings in Bands 6 and 7 through observations of the high-mass starforming region NGC 6334I-MM1. Assuming an excitation temperature of 200 K, its column density was found to be lower than that of methanol by a factor slightly larger than 30.
 +
 +B. Tercero, S. Cuadrado, A. López, N. Brouillet, D. Despois, and J. Cernicharo\\
 +investigated\\
 +**[[https://doi.org/10.1051/0004-6361/201834417|Chemical Segregation of Complex Organic O-bearing Species in Orion KL]]**\\
 +//Astron. Astrophys.// **620**, Art. No. L6 (2018).\\
 +They analyzed the Cycle 0 ALMA science verification data and found ethyl methyl ether besides several other molecules.
  
  
 ---- ----
  
-Contributor(s): H. S. P. Müller; 12, 2017+Contributor(s): H. S. P. Müller; 12, 2017; 07, 2019
  
  
  • molecules/ism/methoxymethanol.txt
  • Last modified: 2020/03/10 09:18
  • by mueller