通过 QUIJOTE 线测量发现 TMC-1 中的 HCCCH_2CCH

R. Fuentetaja, M. Ag'undez, C. Cabezas, B. Tercero, N. Marcelino, J. R. Pardo, P. D. Vicente, J. Cernicharo
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引用次数: 0

摘要

我们首次在太空中探测到了 1,4-五氧化二钒。我们利用 QUIJOTE 线巡天仪在 31-50 GHz 范围内发现了 1,4-五氧化二钒。我们总共观测到了 17 个 J$ = 2 到 13、K_a$ = 0、1 和 2 的跃迁。通过观测到的跃迁,我们推算出该分子的旋转温度为 9.5 pm 0.5 K,柱密度为 (5.0 pm 0.5)times 1012 cm$^$。计算化学研究确定了五种最稳定异构体的能量。异构体($c$-C$_3$H$_3$CCH)的能量比其他异构体高得多,但尚未被探测到。为了更好地理解涉及这些物种的化学反应,我们比较了乙炔基和氰基衍生物。观测到的这些物种的丰度与我们的 TMC-1 化学模型所研究的形成反应的分支比率非常吻合。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Discovery of HCCCH_2CCH in TMC-1 with the QUIJOTE line survey
We present the first detection in space of 1,4-pentadiyne. It has been found towards TMC-1 with the QUIJOTE line survey in the 31-50 GHz range. We observed a total of 17 transitions with $J$ = 2 up to 13 and $K_a$ = 0,1 and 2. The observed transitions allowed us to derive a rotational temperature of 9.5 pm 0.5 K and a column density of (5.0 pm 0.5)times 1012 cm$^ $. This molecule was the last non-cyclic isomer of the C$_5$H$_4$ family that could be detected via radio astronomy. A computational chemistry study was performed to determine the energies of the five most stable isomers. The isomer ($c$-C$_3$H$_3$CCH) has a considerably higher energy than the others, and it has not yet been detected. To better understand the chemical reactions involving these species, we compared the ethynyl and cyano derivatives. The observed abundances of these species are in good agreement with the branching ratios of the formation reactions studied with our chemical model of TMC-1.
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