Show pageOld revisionsBacklinksBack to top This page is read only. You can view the source, but not change it. Ask your administrator if you think this is wrong. ===== On the Cyanohexatriynylide Ion, C7N–, in Space ===== J. Cernicharo, J. R. Pardo, C. Cabezas, M. Agúndez, B. Tercero, N. Marcelino, R. Fuentetaja, M. Guélin, and P. de Vicente\\ reported on the\\ **[[https://doi.org/10.1051/0004-6361/202245816|Discovery of the C<sub>7</sub>N<sup>−</sup> Anion in TMC-1 and IRC +10216]]**\\ //Astron. Astrophys.// **670**, (2023), Art. No. L19.\\ Six transitions with 26 ≤ //J"// ≤ 31 and 17 transitions with 26 ≤ //J"// ≤ 42 were detected toward the dark cloud TMC-1 and the C-rich late-type star CW Leonis, respectively, in the course of two molecular line surveys. The identification relies on quantum-chemical observations as no laboraotory data exist to date, as in the case of C<sub>5</sub>N<sup>−</sup>. The rotational temperature //T//<sub>rot</sub> was fit as 6.0 ± 0.5 K in TMC-1 and as 26.6 ± 1.8 K toward CW Leonis; both values are similar to those of C<sub>5</sub>N<sup>−</sup>. The C<sub>5</sub>N<sup>−</sup> to C<sub>7</sub>N<sup>−</sup> in TMC-1 is ~5, toward CW Leonis ~2.4.\\ \\ ---- Contributor(s): H. S. P. Müller; 02, 2023 ---- molecules/ism/c7n.txt Last modified: 2023/02/20 14:14by mueller