| Literature DB >> 33239826 |
N Marcelino1, M Agúndez1, B Tercero2,3, C Cabezas1, C Bermúdez1, J D Gallego2, P de Vicente2, J Cernicharo1.
Abstract
Using the Yebes 40m radio telescope, we report the detection of a series of seven lines harmonically related with a rotational constant B 0=1295.81581 ± 0.00026 MHz and a distortion constant D 0 = 27.3 ± 0.5 Hz towards the cold dense cloud TMC-1. Ab initio calculations indicate that the best possible candidates are the cations HC5NH+ and NC4NH+. From a comparison between calculated and observed rotational constants and other arguments based on proton affinities and dipole moments, we conclude that the best candidate for a carrier of the observed lines is the protonated cyanodiacetylene cation, HC5NH+. The HC5N/HC5NH+ ratio derived in TMC-1 is 240, which is very similar to the HC3N/HC3NH+ ratio. Results are discussed in the framework of a chemical model for protonated molecules in cold dense clouds.Entities:
Keywords: Astrochemistry; ISM: individual (TMC-1); ISM: molecules; line: identification; molecular data
Year: 2020 PMID: 33239826 PMCID: PMC7116411 DOI: 10.1051/0004-6361/202039251
Source DB: PubMed Journal: Astron Astrophys ISSN: 0004-6361 Impact factor: 5.802