molecules:ism:mesh

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molecules:ism:mesh [2019/05/09 12:36] – muellermolecules:ism:mesh [2019/10/23 22:01] – mueller
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 Methyl mercaptan, or methanethiol, CH<sub>3</sub>SH, was detected in emission with the 7 m Bell Lab telescope toward Sagittarius B2(OH):\\ Methyl mercaptan, or methanethiol, CH<sub>3</sub>SH, was detected in emission with the 7 m Bell Lab telescope toward Sagittarius B2(OH):\\
 R. A. Linke, M. A. Frerking, and P. Thaddeus,\\ R. A. Linke, M. A. Frerking, and P. Thaddeus,\\
-**[[http://adsabs.harvard.edu/abs/1979ApJ...234L.139L|Interstellar methyl mercaptan]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1979ApJ...234L.139L|Interstellar methyl mercaptan]]**\\
 //Astrophys. J.// **232**, L139–L142 (1979).\\ //Astrophys. J.// **232**, L139–L142 (1979).\\
 6 features belonging to several more //J// = 3 –2 and 4 –3 were observed near 75.9 and near 101 GHz. The derived rotational temperature in that source was about 9 K. 6 features belonging to several more //J// = 3 –2 and 4 –3 were observed near 75.9 and near 101 GHz. The derived rotational temperature in that source was about 9 K.
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 reported on the\\ reported on the\\
 **[[https://doi.org/10.1093/mnras/stw457|Detection of CH<sub>3</sub>SH in protostar IRAS 16293-2422]]**\\ **[[https://doi.org/10.1093/mnras/stw457|Detection of CH<sub>3</sub>SH in protostar IRAS 16293-2422]]**\\
-//Mon. Not. R. Astron. Soc.// **458**, 1859–1865 (2000).\\+//Mon. Not. R. Astron. Soc.// **458**, 1859–1865 (2016).\\
 The IRAM 30 m telescope was used to study this solar-type pair of proto-stars at 3 mm. Here, an excitation temperature of 32 ± 4 K was derived. The IRAM 30 m telescope was used to study this solar-type pair of proto-stars at 3 mm. Here, an excitation temperature of 32 ± 4 K was derived.
  
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 Contributor(s): H. S. P. Müller; 10, 2010; 07, 2016 Contributor(s): H. S. P. Müller; 10, 2010; 07, 2016
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  • molecules/ism/mesh.txt
  • Last modified: 2021/05/07 15:54
  • by mueller