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Steps toward Identifying PAHs: A Summary of Some Recent Results
2006
Proceedings of the International Astronomical Union
Based on over two decades of experimental, observational, and theoretical studies by scientists around the world, it is now widely accepted that the composite emission of mixtures of vibrationally-excited PAHs and PAH ions can accommodate the general pattern of band positions, intensities, and profiles observed in the discrete IR emission features of carbon-rich interstellar dust, as well as the variations in those characteristics. These variations provide insight into the detailed nature of
doi:10.1017/s1743921306007459
fatcat:lkwlhoxhgff6bjbqlz6zexraya