molecules:ism:bd-e1cn

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molecules:ism:bd-e1cn [2023/07/27 13:26] – created muellermolecules:ism:bd-e1cn [2023/07/27 13:34] (current) – mueller
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-===== On the Detection of 1-Cyano-1,3-butadiene, H3C(CH)3CN, in Space =====+===== On the Detection of 1-Cyano-1,3-butadiene, H2C(CH)3CN, in Space =====
  
 I. R. Cooke, C. Xue, P. B. Changala, H. T. Shay, A. N. Byrne, Q. Y. Tang, Z. T. P. Fried, K. L. K. Lee, R. A. Loomis, T.Lamberts, A. Remijan, A. M. Burkhardt, E. Herbst, M. C. McCarthy, and B. A. McGuire\\ I. R. Cooke, C. Xue, P. B. Changala, H. T. Shay, A. N. Byrne, Q. Y. Tang, Z. T. P. Fried, K. L. K. Lee, R. A. Loomis, T.Lamberts, A. Remijan, A. M. Burkhardt, E. Herbst, M. C. McCarthy, and B. A. McGuire\\
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 **[[https://doi.org/10.3847/1538-4357/acc584|Detection of Interstellar //E//-1-cyano-1,3-butadiene in GOTHAM Observations of TMC-1]]**\\ **[[https://doi.org/10.3847/1538-4357/acc584|Detection of Interstellar //E//-1-cyano-1,3-butadiene in GOTHAM Observations of TMC-1]]**\\
 //Astrophys. J.// **948**, Art. No. 133 (2023).\\ //Astrophys. J.// **948**, Art. No. 133 (2023).\\
 +The identification was made by stacking data from the GBT line survey that covers ~24.9 GHZ of the 7.9 to 36.4 GHz region. The //E// form of 1-cyano-1,3-butadiene is less abundant than the two detected cyanocyclopentadiene isomers by factors of a few, somewhat depending on the sources of the column densities of the cyclic species.\\
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 +Contributor(s): H. S. P. Müller; 07, 2023
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