This is an old revision of the document!
On HCxN+ in the ISM
J. Cernicharo, C. Cabezas, M. Agúndez, Y. Endo, B. Tercero, N. Marcelino and P. de Vicente
reported on the
QUIJOTE discovery of the cation radicals HC5N+ and HC7N+
Astron. Astrophys. 686, Art. No. L15 (2024).
HC5N+ and HC7N+ were identified through 7 and 8 unblended or slightly blended transitions, respectively with 23/2 ≤ J ≤ 37/2 in the first case and 53/2 ≤ J ≤ 69/2 in the latter. The identifications were made in the course of a molecular line survey of the prototypical cold dark molecular cloud TMC-1 carried out with the Yebes 40 m radio telescope between 31.0 and 50.3 GHz. Trot = 8.5 ± 0.5 K was derived for . The column density of 1-butnyne is about a factor of 15 lower than that of butenyne.
Contributor(s): H. S. P. Müller; 06, 2024