2017
DOI: 10.3847/1538-4357/aa8141
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On the Origin of the 3.3 μm Unidentified Infrared Emission Feature

Abstract: The 3.3 µm unidentified infrared emission feature is commonly attributed to C-H stretching band of aromatic molecules. Astronomical observations have shown that this feature is composed of two separate bands at 3.28 and 3.30 µm and the origin of these two bands is unclear. In this paper, we perform vibrational analyses based on quantum mechanical calculations of 153 organic molecules, including both pure aromatic molecules and molecules with mixed aromatic/olefinic/aliphatic hydridizations. We find that many o… Show more

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Cited by 15 publications
(17 citation statements)
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“…For example, Chiar et al (2013) interpret the 3.28 µm component as the stretching mode of olefinic C-H bonds in amorphous hydrocarbons. The possibility that the 3.30 µm subfeature is due to olefinic C-H stretch is discussed by Sadjadi et al (2017).…”
Section: The 33 μM Bandmentioning
confidence: 99%
See 1 more Smart Citation
“…For example, Chiar et al (2013) interpret the 3.28 µm component as the stretching mode of olefinic C-H bonds in amorphous hydrocarbons. The possibility that the 3.30 µm subfeature is due to olefinic C-H stretch is discussed by Sadjadi et al (2017).…”
Section: The 33 μM Bandmentioning
confidence: 99%
“…The possibility that the 3.30 μm subfeature is due to olefinic C-H stretch is discussed by Sadjadi et al. ( 2017 ).…”
Section: Corresponding Vibrational Modes Of the Uie Featuresmentioning
confidence: 99%
“…Here a modern and advanced molecular chemical bonding and structure theory such as the quantum theory of atoms in molecules should be recalled to assist the interpretation [25][26][27]. [19,28]. Based on this new mathematical analysis we find that:…”
Section: New Results From This Workmentioning
confidence: 99%
“…Experimental infrared spectra of such compounds show naturally broad emission features resembling the astronomical UIE bands (Dischler et al 1983). We are currently undertaking quantum chemistry calculations to study the vibrational modes of MAON-like molecules with the goal of S. Kwok, S. Sadjadi & Y. Zhang testing the hypothesis that MAONs are the chemical carriers of astronomical UIE bands (Sadjadi et al 2015(Sadjadi et al , 2017.…”
Section: Evolved Stars As Sources Of Complex Organicsmentioning
confidence: 99%