molecules:ism:etcn

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molecules:ism:etcn [2019/04/25 13:35] – muellermolecules:ism:etcn [2022/03/17 09:39] (current) – mueller
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 Ethyl cyanide, C<sub>2</sub>H<sub>5</sub>CN, aka propanenitrile, is a fairly prototypical hot core molecule. It was detected first toward OMC-1 and Sgr B2:\\ Ethyl cyanide, C<sub>2</sub>H<sub>5</sub>CN, aka propanenitrile, is a fairly prototypical hot core molecule. It was detected first toward OMC-1 and Sgr B2:\\
 D. R. Johnson, F. J. Lovas, C. A. Gottlieb, E. W. Gottlieb, M. M. Litvak, P. Thaddeus, and M. Guélin,\\ D. R. Johnson, F. J. Lovas, C. A. Gottlieb, E. W. Gottlieb, M. M. Litvak, P. Thaddeus, and M. Guélin,\\
-**[[http://cdsads.u-strasbg.fr/abs/1977ApJ...218..370J|Detection of Interstellar Ethyl Cyanide]]**\\ +**[[https://ui.adsabs.harvard.edu/abs/1977ApJ...218..370J|Detection of Interstellar Ethyl Cyanide]]**\\ 
-//Astrophys. J.// **218**, L370–L376 (1977).+//Astrophys. J.// **218**, L370–L376 (1977).\\
  
 More recently, however, it has also been detected toward a low-mass star-forming region:\\ More recently, however, it has also been detected toward a low-mass star-forming region:\\
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 D. M. Mehringer, J. C. Pearson, J. Keene, and T. G. Philips,\\ D. M. Mehringer, J. C. Pearson, J. Keene, and T. G. Philips,\\
 **[[https://doi.org/10.1086/386357|Detection of Vibrationally Excited Ethyl Cyanide in the Interstellar Medium]]**\\ **[[https://doi.org/10.1086/386357|Detection of Vibrationally Excited Ethyl Cyanide in the Interstellar Medium]]**\\
-//Astrophys. J.// **608**, 306–313 (2004).+//Astrophys. J.// **608**, 306–313 (2004).\\
  
 These states as well as higher vibrational states up to v<sub>12</sub> = 1 at 770 K were detected toward Orion KL by\\ These states as well as higher vibrational states up to v<sub>12</sub> = 1 at 770 K were detected toward Orion KL by\\
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 A. Belloche, H. S. P. Müller, K. M. Menten, P. Schilke, and C. Comito:\\ A. Belloche, H. S. P. Müller, K. M. Menten, P. Schilke, and C. Comito:\\
 **[[https://doi.org/10.1051/0004-6361/201321096|Complex Organic Molecules in the Interstellar Medium: IRAM 30 m Line Survey of Sagittarius B2(N) and (M)]]**\\ **[[https://doi.org/10.1051/0004-6361/201321096|Complex Organic Molecules in the Interstellar Medium: IRAM 30 m Line Survey of Sagittarius B2(N) and (M)]]**\\
-//Astron. Astrophys.// **559**, Art. No. A47 (2013).+//Astron. Astrophys.// **559**, Art. No. A47 (2013).\\
  
 The three <sup>13</sup>C isotopic species have been reported first in observations toward Orion IRc2 by\\ The three <sup>13</sup>C isotopic species have been reported first in observations toward Orion IRc2 by\\
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 H. S. P. Müller, A. Belloche, K. M. Menten, C. Comito, and P. Schilke,\\ H. S. P. Müller, A. Belloche, K. M. Menten, C. Comito, and P. Schilke,\\
 **[[https://doi.org/10.1016/j.jms.2008.03.016|Rotational Spectroscopy of Isotopic Vinyl Cyanide, H<sub>2</sub>C=CH–C≡N, in the Laboratory and in Space]]**,\\ **[[https://doi.org/10.1016/j.jms.2008.03.016|Rotational Spectroscopy of Isotopic Vinyl Cyanide, H<sub>2</sub>C=CH–C≡N, in the Laboratory and in Space]]**,\\
-//J. Mol. Spectrosc.// **250**, 319–325 (2008).+//J. Mol. Spectrosc.// **250**, 319–325 (2008).\\
  
 The detection of the <sup>15</sup>N isotopolog (in Orion KL) was reported first by\\ The detection of the <sup>15</sup>N isotopolog (in Orion KL) was reported first by\\
 L. Margulès, R. Motiyenko, K. Demyk, B. Tercero, J. Cernicharo, M. Sheng, M. Weidmann, J. Gripp, H. Mäder, and J. Demaison,\\ L. Margulès, R. Motiyenko, K. Demyk, B. Tercero, J. Cernicharo, M. Sheng, M. Weidmann, J. Gripp, H. Mäder, and J. Demaison,\\
 **[[https://doi.org/10.1051/0004-6361:200810889|Rotational Spectrum of Deuterated and <sup>15</sup>N Ethyl Cyanides: CH<sub>3</sub>CHDCN and CH<sub>2</sub>DCH<sub>2</sub>CN and of CH<sub>3</sub>CH<sub>2</sub>C<sup>15</sup>N]]**\\ **[[https://doi.org/10.1051/0004-6361:200810889|Rotational Spectrum of Deuterated and <sup>15</sup>N Ethyl Cyanides: CH<sub>3</sub>CHDCN and CH<sub>2</sub>DCH<sub>2</sub>CN and of CH<sub>3</sub>CH<sub>2</sub>C<sup>15</sup>N]]**\\
-//Astron. Astrophys.// **559**, Art. No. A47 (2013).\\+//Astron. Astrophys.// **493**, 565 (2009).\\
 The isotopolog was also detected in Sagittarius B2(N2), the northern, secondary hot-core of Sgr B2(N), by\\ The isotopolog was also detected in Sagittarius B2(N2), the northern, secondary hot-core of Sgr B2(N), by\\
 A. Belloche, H. S. P. Müller, R. T. Garrod, and K. M. Menten,\\ A. Belloche, H. S. P. Müller, R. T. Garrod, and K. M. Menten,\\
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 Contributor(s): H. S. P. Müller; 07, 2004; 03/04 2007; 10, 2010; 06, 2016 Contributor(s): H. S. P. Müller; 07, 2004; 03/04 2007; 10, 2010; 06, 2016
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