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星际1-氰基芘的检测:一种四环多环芳烃。

Detection of interstellar 1-cyanopyrene: A four-ring polycyclic aromatic hydrocarbon.

作者信息

Wenzel Gabi, Cooke Ilsa R, Changala P Bryan, Bergin Edwin A, Zhang Shuo, Burkhardt Andrew M, Byrne Alex N, Charnley Steven B, Cordiner Martin A, Duffy Miya, Fried Zachary T P, Gupta Harshal, Holdren Martin S, Lipnicky Andrew, Loomis Ryan A, Shay Hannah Toru, Shingledecker Christopher N, Siebert Mark A, Stewart D Archie, Willis Reace H J, Xue Ci, Remijan Anthony J, Wendlandt Alison E, McCarthy Michael C, McGuire Brett A

机构信息

Department of Chemistry, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.

Department of Chemistry, University of British Columbia, Vancouver, BC V6T 1Z1, Canada.

出版信息

Science. 2024 Nov 15;386(6723):810-813. doi: 10.1126/science.adq6391. Epub 2024 Oct 24.

Abstract

Polycyclic aromatic hydrocarbons (PAHs) are organic molecules containing adjacent aromatic rings. Infrared emission bands show that PAHs are abundant in space, but only a few specific PAHs have been detected in the interstellar medium. We detected 1-cyanopyrene, a cyano-substituted derivative of the related four-ring PAH pyrene, in radio observations of the dense cloud TMC-1, using the Green Bank Telescope. The measured column density of 1-cyanopyrene is [Formula: see text] cm, from which we estimate that pyrene contains up to 0.1% of the carbon in TMC-1. This abundance indicates that interstellar PAH chemistry favors the production of pyrene. We suggest that some of the carbon supplied to young planetary systems is carried by PAHs that originate in cold molecular clouds.

摘要

多环芳烃(PAHs)是含有相邻芳环的有机分子。红外发射带表明PAHs在宇宙空间中含量丰富,但在星际介质中仅检测到少数特定的PAHs。我们使用绿岸望远镜对致密云TMC-1进行了射电观测,检测到了1-氰基芘,它是相关四环PAH芘的氰基取代衍生物。测得的1-氰基芘柱密度为[公式:见原文]厘米,由此我们估计芘在TMC-1中所含碳的比例高达0.1%。这一丰度表明星际PAH化学过程有利于芘的生成。我们认为,一些输送到年轻行星系统的碳是由源自寒冷分子云的PAHs携带的。

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