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--- molecules:ism:c5n-minus [2019/05/09 12:41] – mueller
+++ molecules:ism:c5n-minus [2020/09/23 17:06] (current) – mueller
@@ Line 12: / Line 12: @@
 An additional line, U33332.3, reported by\\
 K. Kawaguchi, Y. Kasai, S.-I. Ishikawa, and N. Kaifu,\\
-**[[http://cdsads.u-strasbg.fr/abs/1995PASJ...47..853K|A Spectral-Line Survey Observation of IRC +10216 between 28 and 50 GHz]]**\\
+**[[https://ui.adsabs.harvard.edu/abs/1995PASJ...47..853K|A Spectral-Line Survey Observation of IRC +10216 between 28 and 50 GHz]]**\\
 //Publ. Astron. Soc. Japan// **47**, 853–876 (1995),\\
 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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