molecules:ism:hcs-plus

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molecules:ism:hcs-plus [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:hcs-plus [2019/10/21 17:27] (current) – mueller
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 The thioformyl cation, HCS<sup>+</sup>, has been observed in the ISM prior to the laboratory by\\ The thioformyl cation, HCS<sup>+</sup>, has been observed in the ISM prior to the laboratory by\\
 P. Thaddeus, M. Guélin, and R. A. Linke,\\ P. Thaddeus, M. Guélin, and R. A. Linke,\\
-**[[http://cdsads.u-strasbg.fr/abs/1981ApJ...246L..41T|Three New 'Nonterrestrial' Molecules]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1981ApJ...246L..41T|Three New 'Nonterrestrial' Molecules]]**\\
 //Astrophys. J.// **246**, L41–L45 (1981).\\ //Astrophys. J.// **246**, L41–L45 (1981).\\
 The //J// = 2 – 1 transition near 85.3 GHz was detected toward the hot-core sources Orion KL, Sgr B2(OH), and DR 21 as well as toward the dense cold cloud TMC-1. In addition, the 3 – 2, 5 – 4, and 6 – 5 transitions were also detected in Orion KL. The //J// = 2 – 1 transition near 85.3 GHz was detected toward the hot-core sources Orion KL, Sgr B2(OH), and DR 21 as well as toward the dense cold cloud TMC-1. In addition, the 3 – 2, 5 – 4, and 6 – 5 transitions were also detected in Orion KL.
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 The molecular cation was also detected in several translucent molecular clouds by\\ The molecular cation was also detected in several translucent molecular clouds by\\
 B. E. Turner,\\ B. E. Turner,\\
-**[[http://cdsads.u-strasbg.fr/abs/1996ApJ...461..246T|The Physics and Chemistry of Small Translucent Molecular Clouds. VI. Organo-Sulfur Species]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1996ApJ...461..246T|The Physics and Chemistry of Small Translucent Molecular Clouds. VI. Organo-Sulfur Species]]**\\
 //Astrophys. J.// **416**, 246–264 (1996) //Astrophys. J.// **416**, 246–264 (1996)
  
 The 7 – 6, and 8 – 7 transitions were detected in a PDR by\\ The 7 – 6, and 8 – 7 transitions were detected in a PDR by\\
 S. Leurini, R. Rolffs, S. Thorwirth, B. Parise, P. Schilke, C. Comito, F. Wyrowski, R. Güsten, P. Bergman, K. M. Menten, and L.-Å. Nyman,\\ S. Leurini, R. Rolffs, S. Thorwirth, B. Parise, P. Schilke, C. Comito, F. Wyrowski, R. Güsten, P. Bergman, K. M. Menten, and L.-Å. Nyman,\\
-**[[http://dx.doi.org/10.1051/0004-6361:20065555|APEX 1 mm Line Survey of the Orion Bar]]**\\+**[[https://doi.org/10.1051/0004-6361:20065555|APEX 1 mm Line Survey of the Orion Bar]]**\\
 //Astron. Astrophys.// **454**, L47–L50 (2006) //Astron. Astrophys.// **454**, L47–L50 (2006)
  
 A. Fuente, J. Cernicharo, E. Roueff, M. Gerin, J. Pety, N. Marcelino, R. Bachiller, B. Lefloch, O. Roncero, and A. Aguado,\\ A. Fuente, J. Cernicharo, E. Roueff, M. Gerin, J. Pety, N. Marcelino, R. Bachiller, B. Lefloch, O. Roncero, and A. Aguado,\\
 studied the\\ studied the\\
-**[[http://dx.doi.org/10.1051/0004-6361/201628285|Ionization Fraction and the Enhanced Sulfur Chemistry in Barnard 1]]**\\+**[[https://doi.org/10.1051/0004-6361/201628285|Ionization Fraction and the Enhanced Sulfur Chemistry in Barnard 1]]**\\
 //Astron. Astrophys.// **593**, Art. No. A94 (2016).\\ //Astron. Astrophys.// **593**, Art. No. A94 (2016).\\
 They used the IRAM 30 m telescope for a molecular line survey at 3, 2, and 1.3 mm. The //J// = 3 – 2 transition of DCS<sup>+</sup> at 108.108 GHz was detected in emission. An LVG analysis suggests a D/H ratio of almost 0.1 in the region in which the DCS<sup>+</sup> emission was detected. They used the IRAM 30 m telescope for a molecular line survey at 3, 2, and 1.3 mm. The //J// = 3 – 2 transition of DCS<sup>+</sup> at 108.108 GHz was detected in emission. An LVG analysis suggests a D/H ratio of almost 0.1 in the region in which the DCS<sup>+</sup> emission was detected.
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 A. Potapov, Á. Sánchez-Monge, P. Schilke, U. U. Graf, T. Möller, and S. Schlemmer\\ A. Potapov, Á. Sánchez-Monge, P. Schilke, U. U. Graf, T. Möller, and S. Schlemmer\\
 reported almost at the same time on the detection of the same transition in their search for\\ reported almost at the same time on the detection of the same transition in their search for\\
-**[[http://dx.doi.org/10.1051/0004-6361/201628426|The CO–H<sub>2</sub> van der Waals complex and complex organic molecules in cold molecular clouds: A TMC-1C survey]]**\\+**[[https://doi.org/10.1051/0004-6361/201628426|The CO–H<sub>2</sub> van der Waals complex and complex organic molecules in cold molecular clouds: A TMC-1C survey]]**\\
 //Astron. Astrophys.// **594**, Art. No. A117 (2016).\\ //Astron. Astrophys.// **594**, Art. No. A117 (2016).\\
 The IRAM 30 m telescope was used once more. The IRAM 30 m telescope was used once more.
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 Contributor(s): H. S. P. Müller; 12, 2003; 09, 2011; 11, 2016 Contributor(s): H. S. P. Müller; 12, 2003; 09, 2011; 11, 2016
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