| Literature DB >> 33737489 |
Ryan A Loomis1, Andrew M Burkhardt2, Brett A McGuire3,1,2, Kin Long Kelvin Lee4,2, Christopher N Shingledecker5,6,7, Steven B Charnley8, Ilsa R Cooke9, Martin A Cordiner8,10, Eric Herbst11,12, Sergei Kalenskii13, Mark A Siebert12, Eric R Willis11, Ci Xue11, Anthony J Remijan1, Michael C McCarthy2.
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.Entities:
Year: 2021 PMID: 33737489 DOI: 10.1126/science.abb7535
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728