molecules:ism:c5n-minus

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molecules:ism:c5n-minus [2019/10/23 22:06] muellermolecules:ism:c5n-minus [2020/09/23 17:06] (current) mueller
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 //Publ. Astron. Soc. Japan// **47**, 853–876 (1995),\\ //Publ. Astron. Soc. Japan// **47**, 853–876 (1995),\\
 is, at least in part, due to C<sub>5</sub>N<sup>–</sup>.\\ is, at least in part, due to C<sub>5</sub>N<sup>–</sup>.\\
-This anion is isolelectronic to C<sub>6</sub>H<sup>–</sup> which was the first molecular anion to be detected in space. In addition, it is a sibling of the recently detected C<sub>3</sub>N<sup>–</sup>.+This anion is isolelectronic to C<sub>6</sub>H<sup>–</sup> which was the first molecular anion to be detected in space. In addition, it is a sibling of the recently detected C<sub>3</sub>N<sup>–</sup>.\\ 
 + 
 +Meanwhile,\\ 
 +J. Cernicharo, N. Marcelino, J. R. Pardo, M. Agúndez, B. Tercero, P. de Vicente, C. Cabezas, and C. Bermúdez\\ 
 +reported on\\ 
 +**[[https://doi.org/10.1051/0004-6361/202039231|Interstellar nitrile anions: Detection of C<sub>3</sub>N<sup>–</sup> and C<sub>5</sub>N<sup>–</sup> in TMC-1]]**\\ 
 +//Astron. Astrophys.// **641**, Art. No. L9 (2020).\\
  
  
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-Contributor(s): H. S. P. Müller; 10, 2008+Contributor(s): H. S. P. Müller; 10, 2008; 09, 2020
  
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