论文标题

高度极性五元环氰基戊二烯的星际检测

Interstellar Detection of the Highly Polar Five-Membered Ring Cyanocyclopentadiene

论文作者

McCarthy, Michael C., Lee, Kin Long Kelvin, Loomis, Ryan A., Burkhardt, Andrew M., Shingledecker, Christopher N., Charnley, Steven B., Cordiner, Martin A., Herbst, Eric, Kalenskii, Sergei, Willis, Eric R., Xue, Ci, Remijan, Anthony J., McGuire, Brett A.

论文摘要

就像六元环一样,有机化学中的五个元素无处不在,经常充当大分子的基础,包括许多生化重要性。 From a combination of laboratory rotational spectroscopy and a sensitive spectral line survey in the radio band toward the starless cloud core TMC-1, we report the astronomical detection of 1-cyano-1,3-cyclopentadiene, $c$-C$_5$H$_5$CN}, a highly polar, cyano derivative of cyclopentadiene, $ c $ -c $ _5 $ h $ _6 $。 $ c $ -c $ _5 $ h $ _5 $ cn}的派生丰度远远超过天文学模型所预测的,这些模型可以很好地繁殖许多碳链。这一发现意味着可能需要考虑重要的生产机制或大量芳香材料储层。显然缺乏与其密切相关的异构体2-Cyano-1,3-循环丙烯,可能是由于其较低的稳定性而引起的,或者表明形成1-氰基异构体的更选择性途径,也许是从千合性前体开始的。根据天文学发现,讨论了吡咯和吡啶等N型型细胞(例如吡咯和吡啶的)。

Much like six-membered rings, five-membered rings are ubiquitous in organic chemistry, frequently serving as the building blocks for larger molecules, including many of biochemical importance. From a combination of laboratory rotational spectroscopy and a sensitive spectral line survey in the radio band toward the starless cloud core TMC-1, we report the astronomical detection of 1-cyano-1,3-cyclopentadiene, $c$-C$_5$H$_5$CN}, a highly polar, cyano derivative of cyclopentadiene, $c$-C$_5$H$_6$. The derived abundance of $c$-C$_5$H$_5$CN} is far greater than predicted from astrochemical models which well reproduce the abundance of many carbon chains. This finding implies either an important production mechanism or a large reservoir of aromatic material may need to be considered. The apparent absence of its closely-related isomer, 2-cyano-1,3-cyclopentadiene, may arise from its lower stability or be indicative of a more selective pathway for formation of the 1-cyano isomer, perhaps one starting from acyclic precursors. The absence of N-heterocycles such as pyrrole and pyridine is discussed in light of the astronomical finding.

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