UNIDENTIFIED INFRARED EMISSION BANDS: PAHs or MAONs?

被引:78
|
作者
Kwok, Sun [1 ]
Zhang, Yong [1 ]
机构
[1] Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2013年 / 771卷 / 01期
关键词
infrared: ISM; ISM: lines and bands; ISM: molecules; planetary nebulae: general; POLYCYCLIC AROMATIC-HYDROCARBONS; HYDROGENATED AMORPHOUS-CARBON; DIFFUSE INTERSTELLAR-MEDIUM; MU-M EMISSION; LABORATORY SIMULATION; COMPOSITE QCC; SMALL GRAINS; SPECTRA; FEATURES; DUST;
D O I
10.1088/0004-637X/771/1/5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We suggest that the carrier of the unidentified infrared emission (UIE) bands is an amorphous carbonaceous solid with mixed aromatic/aliphatic structures, rather than free-flying polycyclic aromatic hydrocarbon molecules. Through spectral fittings of the astronomical spectra of the UIE bands, we show that a significant amount of the energy is emitted by the aliphatic component, implying that aliphatic groups are an essential part of the chemical structure. Arguments in favor of an amorphous, solid-state structure rather than a gas-phase molecule as a carrier of the UIE are also presented.
引用
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页数:9
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