在太空和实验室发现亚氨基戊二烯,HNC5⋆

IF 5.4 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2024-08-15 DOI:10.1051/0004-6361/202451319
R. Fuentetaja, C. Cabezas, Y. Endo, M. Agúndez, B. Tercero, N. Marcelino, P. de Vicente, J. Cernicharo
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引用次数: 0

摘要

我们报告在 TMC-1 中发现了 HNC5。发现了六条谐波关系线,量子数从 J = 12-11 到 J = 17-16。这些线可以用线性分子的标准频率关系(B = 1361.75034 ± 0.00033 MHz 和 D = 32.2 ± 0.7 Hz)重现。通过高水平的理论 ab initio 计算,对可能的候选分子进行了研究,从而将载流子确定为亚氨基戊二烯。由于观测到的 B 与 HNC5 的计算值十分吻合,我们在实验室中对其进行了搜索,并观测到了 J = 5-4 到 7-6 的转变。得出的旋转常数和畸变常数分别为 1361.74998 ± 0.00040 MHz 和 26.5 ± 5.5 Hz。因此,我们断定在 TMC-1 中发现的线的载体是 HNC5。该物种的计算偶极矩为 7.7 D,得出的柱密度为 (1.3 ± 0.2) × 1010 cm-2。我们利用新的 QUIJOTE 数据改进了之前对 HC4NC 的观测,发现 HC4NC/HNC5 的丰度比为 10 ± 2。HC5N 及其两种异构体 HC4NC 和 HNC5 的丰度比分别为 500 ± 80 和 5100 ± 800。这些丰度比比 HC3N 同等异构体的丰度比高出 ∼ 10 倍。如果采用类似于较小物种 C3HN 同分异构体的化学结构,化学模型就能很好地再现观测到的丰度。HNC5 和 HC4NC 的形成源于阳离子 HC5NH+ 和 HC4NCH+ 与电子的离解重组。
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Space and laboratory discovery of iminopentadienylidene, HNC5⋆
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+.
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
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.
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