This shows you the differences between two versions of the page.
Both sides previous revision Previous revision | Last revisionBoth sides next revision |
molecules:ism:c3n-minus [2019/10/22 17:08] – mueller | molecules:ism:c3n-minus [2020/09/23 17:04] – mueller |
---|
//Astrophys. J.// **677**, 1132–1139 (2008).\\ | //Astrophys. J.// **677**, 1132–1139 (2008).\\ |
This anion is isolelectronic to C<sub>4</sub>H<sup>–</sup>. Besides the presently more common C<sub>2n</sub>H<sup>–</sup> family, it is the first member of a second family of anions detected in space, C<sub>2n–1</sub>N<sup>–</sup>.\\ | This anion is isolelectronic to C<sub>4</sub>H<sup>–</sup>. Besides the presently more common C<sub>2n</sub>H<sup>–</sup> family, it is the first member of a second family of anions detected in space, C<sub>2n–1</sub>N<sup>–</sup>.\\ |
It was searched for, but not found in TMC-1. | It was searched for, but not found in TMC-1.\\ |
| |
| 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).\\ |
| |
| |
---- | ---- |
| |
Contributor(s): H. S. P. Müller; 4, 2008 | Contributor(s): H. S. P. Müller; 04, 2008; 09, 2020 |
| |
---- | ---- |
| |
| |