Natural SciencesAstronomyPhysicsAtmospheric ChemistryRadio AstronomySpectroscopyInterstellar Absorption LinesInterstellar ChemistryInterstellar MoleculesMolecular CloudsMolecular SpectroscopyRadio SpectroscopyAromatic HydrocarbonsInterstellar HydrocarbonsInterstellar Molecule IdentificationMolecular Cloud ObservationsPolycyclic Aromatic Hydrocarbon AnalysisPolycyclic Aromatic Hydrocarbon EmissionPolycyclic Aromatic HydrocarbonsSpectroscopy Of Interstellar Molecules
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.
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Observation of Gravitational Waves from a Binary Black Hole Merger
B. P. Abbott, R. Abbott, T. D. Abbott et al. · Physical Review Letters · 2016 · 14.3K citations · Full text
Natural Sciences, Astronomy, Physics +15