molecules:ism:hc7n

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molecules:ism:hc7n [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:hc7n [2019/10/24 09:48] – mueller
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 H. W. Kroto, C. Kirby, D. R. M. Walton, L. W. Avery, N. W. Broten, J. M. MacLeod, and T. Oka,\\ H. W. Kroto, C. Kirby, D. R. M. Walton, L. W. Avery, N. W. Broten, J. M. MacLeod, and T. Oka,\\
-**[[http://cdsads.u-strasbg.fr/abs/1978ApJ...219L.133K|The Detection of Cyanohexatriyne, H(C≡C)<sub>3</sub>CN, in Heile's Cloud 2]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1978ApJ...219L.133K|The Detection of Cyanohexatriyne, H(C≡C)<sub>3</sub>CN, in Heile's Cloud 2]]**\\
 //Astrophys. J.// **219**, L133–L137 (1978)\\ //Astrophys. J.// **219**, L133–L137 (1978)\\
 reported the first detection of this cyanopolyyne in two transitions (//J// = 9 – 8 and 21 – 20 near 10.15 and 23.69 GHz, respectively) in Heile's Cloud 2 employing the 46 m radio telecope of the Algonquin Radio Observatory. reported the first detection of this cyanopolyyne in two transitions (//J// = 9 – 8 and 21 – 20 near 10.15 and 23.69 GHz, respectively) in Heile's Cloud 2 employing the 46 m radio telecope of the Algonquin Radio Observatory.
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 More recently, the Effelsberg 100 m telecope was used to study the circumstellar shell of the famous carbon star CW Leo:\\ More recently, the Effelsberg 100 m telecope was used to study the circumstellar shell of the famous carbon star CW Leo:\\
 G. Winnewisser and C. M. Walmsley,\\ G. Winnewisser and C. M. Walmsley,\\
-**[[http://cdsads.u-strasbg.fr/abs/1978A%26A....70L..37W|The Detection of HC<sub>5</sub>N and HC<sub>7</sub>N in IRC +10216]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1978A%26A....70L..37W|The Detection of HC<sub>5</sub>N and HC<sub>7</sub>N in IRC +10216]]**\\
 //Astron. Astrophys.// **70**, L37–L39 (1978).\\ //Astron. Astrophys.// **70**, L37–L39 (1978).\\
 The //J// = 21 – 10 transition near 23.688 GHz was detected for the larger polyyne. The //J// = 21 – 10 transition near 23.688 GHz was detected for the larger polyyne.
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 The molecule has also been detected with the Effelsberg 100 m telescope in the circumstellar envelope of the carbon-rich post-AGB star V1610 Cyg, which is somewhat better known as CRL 2688, by\\ The molecule has also been detected with the Effelsberg 100 m telescope in the circumstellar envelope of the carbon-rich post-AGB star V1610 Cyg, which is somewhat better known as CRL 2688, by\\
 Nguyen-Q-Rieu, D. Graham, and V. Bujarrabal,\\ Nguyen-Q-Rieu, D. Graham, and V. Bujarrabal,\\
-**[[http://cdsads.u-strasbg.fr/abs/1984A%26A...138L...5N|Ammonia and Cyanotriacetylene in the Envelopes of CRL 2688 and IRC +10216]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1984A%26A...138L...5N|Ammonia and Cyanotriacetylene in the Envelopes of CRL 2688 and IRC +10216]]**\\
 //Astron. Astrophys.// **138**, L5–L8 (1984). //Astron. Astrophys.// **138**, L5–L8 (1984).
  
 G. Langston and B. E. Turner described the\\ G. Langston and B. E. Turner described the\\
-**[[http://dx.doi.org/10.1086/511332|Detection of <sup>13</sup>C Isotopomers of the Molecule HC<sub>7</sub>N]]**\\+**[[https://doi.org/10.1086/511332|Detection of <sup>13</sup>C Isotopomers of the Molecule HC<sub>7</sub>N]]**\\
 //Astrophys. J.// **658**, 455–461 (2007).\\ //Astrophys. J.// **658**, 455–461 (2007).\\
 They searched for the //J// = 12 – 11 and 13 – 12 transitions in TMC-1 using the GBT 100 m telescope. No individual isotopomer was found. Instead, a barely significant signal was obtained by averaging all observations. They searched for the //J// = 12 – 11 and 13 – 12 transitions in TMC-1 using the GBT 100 m telescope. No individual isotopomer was found. Instead, a barely significant signal was obtained by averaging all observations.
  
 DC<sub>7</sub>N and (individually) 6 of the 7 <sup>13</sup>C isotopomers were detected in the study\\ DC<sub>7</sub>N and (individually) 6 of the 7 <sup>13</sup>C isotopomers were detected in the study\\
-**[[http://dx.doi.org/10.1093/mnras/stx2972|Detection of HC<sub>5</sub>N and HC<sub>7</sub>N Isotopologues in TMC-1 with the Green Bank Telescope]]**\\+**[[https://doi.org/10.1093/mnras/stx2972|Detection of HC<sub>5</sub>N and HC<sub>7</sub>N Isotopologues in TMC-1 with the Green Bank Telescope]]**\\
 //Mon. Not. R. Astron. Soc.// **474**, 5068–5075 (2018); by\\ //Mon. Not. R. Astron. Soc.// **474**, 5068–5075 (2018); by\\
 A. M. Burkhardt, E. Herbst, S. V. Kalenskii, M. C. McCarthy, A. J. Remijan, and B. A. McGuire. A. M. Burkhardt, E. Herbst, S. V. Kalenskii, M. C. McCarthy, A. J. Remijan, and B. A. McGuire.
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 Contributor(s): H. S. P. Müller; 04, 2012; 01, 2018. Contributor(s): H. S. P. Müller; 04, 2012; 01, 2018.
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  • molecules/ism/hc7n.txt
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