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Titlebook: Dusty Objects in the Universe; Proceedings of the F E. Bussoletti,A. A. Vittone Conference proceedings 1990 Kluwer Academic Publishers 1990

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Cross-Cultural Web Usability Modeltest infrared astronomical objects. Actually, the intensity of the 3.3 µm feature (relative to the total far infrared radiation) increases in the most diffuse and less UV-excited regions of the interstellar medium.
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Shuichi Kurabayashi,Hiroki Hanaokaed at 340, 270, and, less distinct, at 220 nm. One of these features may be related to the known 368 nm transition of C.. It thus appears that at high quenching gas pressures C. is produced along with the carbon dust.
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The Infrared Interstellar Emission Features from the higher spectral resolution and higher sensitivity currently available. Laboratory work on identification of the feature emitting material is abo reviewed, and different candidate materials for the features are compared.
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Yan Zhuang,Guoliang Li,Jianhua Fengesults have implications for the role of polycyclic aromatic hydrocarbons in promoting surface reactions of Si. and other atomic ions in interstellar environments, both in the gas phase and on graphitic grains.
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