R. Fuentetaja, C. Cabezas, Y. Endo, M. Agúndez, B. Tercero, N. Marcelino, P. de Vicente, J. Cernicharo
{"title":"Space and laboratory discovery of iminopentadienylidene, HNC5⋆","authors":"R. Fuentetaja, C. Cabezas, Y. Endo, M. Agúndez, B. Tercero, N. Marcelino, P. de Vicente, J. Cernicharo","doi":"10.1051/0004-6361/202451319","DOIUrl":null,"url":null,"abstract":"We report the discovery of HNC<sub>5<sub/> in TMC-1. Six lines have been found in harmonic relation, with quantum numbers <i>J<i/> = 12−11 up to <i>J<i/> = 17−16. The lines can be reproduced with the standard frequency relation for linear molecules with <i>B<i/> = 1361.75034 ± 0.00033 MHz and <i>D<i/> = 32.2 ± 0.7 Hz. The assignment of the carrier to iminopentadienylidene was achieved through examining the possible candidates at a high level of theoretical ab initio calculations. Motivated by the good agreement between the observed <i>B<i/> and the calculated value for HNC<sub>5<sub/>, we searched for it in the laboratory and observed the transitions <i>J<i/> = 5−4 to 7−6. The derived rotational and distortion constants are 1361.74998 ± 0.00040 MHz and 26.5 ± 5.5 Hz, respectively. Hence, we solidly conclude that the carrier of the lines found in TMC-1 is HNC<sub>5<sub/>. The calculated dipole moment for this species is 7.7 D and the derived column density is (1.3 ± 0.2) × 10<sup>10<sup/> cm<sup>−2<sup/>. We used the new QUIJOTE data to improve previous observations of HC<sub>4<sub/>NC and found that the abundance ratio HC<sub>4<sub/>NC/HNC<sub>5<sub/> is 10 ± 2. The abundance ratio of HC<sub>5<sub/>N and its two isomers HC<sub>4<sub/>NC and HNC<sub>5<sub/> is 500 ± 80 and 5100 ± 800, respectively. These abundance ratios are higher by a factor of ∼10 than those of the equivalent isomers of HC<sub>3<sub/>N. Chemical models reproduce the observed abundances reasonably well when a chemistry similar to that of the smaller species C<sub>3<sub/>HN isomers is adopted. The formation of HNC<sub>5<sub/> and HC<sub>4<sub/>NC arises from the dissociative recombination with electrons of the cations HC<sub>5<sub/>NH<sup>+<sup/> and HC<sub>4<sub/>NCH<sup>+<sup/>.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":null,"pages":null},"PeriodicalIF":5.4000,"publicationDate":"2024-08-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1051/0004-6361/202451319","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
We report the discovery of HNC5 in TMC-1. Six lines have been found in harmonic relation, with quantum numbers J = 12−11 up to J = 17−16. The lines can be reproduced with the standard frequency relation for linear molecules with B = 1361.75034 ± 0.00033 MHz and D = 32.2 ± 0.7 Hz. The assignment of the carrier to iminopentadienylidene was achieved through examining the possible candidates at a high level of theoretical ab initio calculations. Motivated by the good agreement between the observed B and the calculated value for HNC5, we searched for it in the laboratory and observed the transitions J = 5−4 to 7−6. The derived rotational and distortion constants are 1361.74998 ± 0.00040 MHz and 26.5 ± 5.5 Hz, respectively. Hence, we solidly conclude that the carrier of the lines found in TMC-1 is HNC5. The calculated dipole moment for this species is 7.7 D and the derived column density is (1.3 ± 0.2) × 1010 cm−2. We used the new QUIJOTE data to improve previous observations of HC4NC and found that the abundance ratio HC4NC/HNC5 is 10 ± 2. The abundance ratio of HC5N and its two isomers HC4NC and HNC5 is 500 ± 80 and 5100 ± 800, respectively. These abundance ratios are higher by a factor of ∼10 than those of the equivalent isomers of HC3N. Chemical models reproduce the observed abundances reasonably well when a chemistry similar to that of the smaller species C3HN isomers is adopted. The formation of HNC5 and HC4NC arises from the dissociative recombination with electrons of the cations HC5NH+ and HC4NCH+.
期刊介绍:
Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.