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通过光谱匹配滤波检测两种星际多环芳烃。

Detection of two interstellar polycyclic aromatic hydrocarbons via spectral matched filtering.

机构信息

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

National Radio Astronomy Observatory, Charlottesville, VA 22903, USA.

出版信息

Science. 2021 Mar 19;371(6535):1265-1269. doi: 10.1126/science.abb7535.

Abstract

Unidentified infrared emission bands are ubiquitous in many astronomical sources. These bands are widely, if not unanimously, attributed to collective emissions from polycyclic aromatic hydrocarbon (PAH) molecules, yet no single species of this class has been identified in space. Using spectral matched filtering of radio data from the Green Bank Telescope, we detected two nitrile-group-functionalized PAHs, 1- and 2-cyanonaphthalene, in the interstellar medium. Both bicyclic ring molecules were observed in the TMC-1 molecular cloud. In this paper, we discuss potential in situ gas-phase PAH formation pathways from smaller organic precursor molecules.

摘要

在许多天文源中,普遍存在无法识别的红外发射带。这些带广泛存在,如果不是普遍存在的话,归因于多环芳烃(PAH)分子的集体发射,但在太空中尚未识别出此类物质的单一物种。使用绿岸望远镜的射电数据的光谱匹配滤波,我们在星际介质中检测到两种腈基官能化的 PAH,1-和 2-氰基萘。这两种双环分子都在 TMC-1 分子云中被观察到。在本文中,我们讨论了从小的有机前体分子到气相 PAH 的潜在原位形成途径。

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