molecules:ism:mesh

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molecules:ism:mesh [2019/02/25 22:38] – external edit 127.0.0.1molecules: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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 Much higher rotational temperatures (about 70 K) were derived in a 3, 2, and 1 mm line survey carried out with SEST:\\ Much higher rotational temperatures (about 70 K) were derived in a 3, 2, and 1 mm line survey carried out with SEST:\\
 E. Gibb, A. Nummelin, W. M. Irvine, D. C. B. Whittet, and P. Bergman,\\ E. Gibb, A. Nummelin, W. M. Irvine, D. C. B. Whittet, and P. Bergman,\\
-**[[http://dx.doi.org/10.1086/317805|Chemistry of the Organic-Rich Hot Core G327.3–0.6]]**\\+**[[https://doi.org/10.1086/317805|Chemistry of the Organic-Rich Hot Core G327.3–0.6]]**\\
 //Astrophys. J.// **545**, 309–326 (2000). //Astrophys. J.// **545**, 309–326 (2000).
  
 L. Majumdar, P. Gratier, T. Vidal, V. Wakelam, J.-C. Loison, K. M. Hickson, and E. Caux,\\ L. Majumdar, P. Gratier, T. Vidal, V. Wakelam, J.-C. Loison, K. M. Hickson, and E. Caux,\\
 reported on the\\ reported on the\\
-**[[http://dx.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.
  
 H. S. P. Müller, A. Belloche, L.-H. Xu, R. M. Lees, R. T. Garrod, A. Walters, J. van Wijngaarden, F. Lewen, S. Schlemmer, and K. M. Menten,\\ H. S. P. Müller, A. Belloche, L.-H. Xu, R. M. Lees, R. T. Garrod, A. Walters, J. van Wijngaarden, F. Lewen, S. Schlemmer, and K. M. Menten,\\
 reported on\\ reported on\\
-**[[http://dx.doi.org/10.1051/0004-6361/201527470|Exploring molecular complexity with ALMA (EMoCA): Alkanethiols and alkanols in Sagittarius B2(N2)]]**\\+**[[https://doi.org/10.1051/0004-6361/201527470|Exploring molecular complexity with ALMA (EMoCA): Alkanethiols and alkanols in Sagittarius B2(N2)]]**\\
 //Astron. Astrophys.// **587**, Art. No. A92 (2016).\\ //Astron. Astrophys.// **587**, Art. No. A92 (2016).\\
 A line survey of Sgr B2(N) was carried out with ALMA at 3 mm. CH<sub>3</sub>SH was not only detected in its ground vibrational state, but also in its first torsionally excited state, even though the CH<sub>3</sub>OH/CH<sub>3</sub>SH ratio was only about 120. These authors derived a rotational temperature of 180 K in this source. A line survey of Sgr B2(N) was carried out with ALMA at 3 mm. CH<sub>3</sub>SH was not only detected in its ground vibrational state, but also in its first torsionally excited state, even though the CH<sub>3</sub>OH/CH<sub>3</sub>SH ratio was only about 120. These authors derived a rotational temperature of 180 K in this source.
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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