Titlebook: Galactic and Extragalactic Infrared Spectroscopy; Proceedings of the X M. F. Kessler,J. P. Phillips Conference proceedings 1984 D. Reidel P

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中和

The Genetic Aspects of Facial Abnormalities,stressed, rather than those expected from more homogeneous components such as silicates, graphite, or amorphous carbon since these have been discussed in considerable detail elsewhere (e.g. Kr?tschmer and Huffman, 1979, Knacke and Kr?tschmer, 1980, Day, 1979, Borghesi et al., 1983 and references the

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TOXIN

GROWL

Neven Vr?ek,?eljko Dobrovi?,Dragutin KermekMoreover, infrared observations have shown GMCs to be the primary sites of star birth in our galaxy. Indeed, molecular-line observations of these clouds have given us the first detailed glimpses into the physical processes associated with the earliest stages of stellar evolution and perhaps star for

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Ccu106

Absorption and Emission Characteristics of Interstellar Dust. Thus, moderate resolution spectroscopy of the interstellar medium offers unique evidence about the molecules in the condensed and gaseous phases and their distribution. It is the purpose of this paper to discuss the spectral properties of the condensed phase. However, in the astrophysical literatu

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極少

Formation of Molecules on Dustlity and surface mobility are presented, and the implications for interstellar chemistry are briefly explored. Reactions at the surfaces of oxide grains are reviewed, and their contributions to sulphur-bearing molecules, and hydroxides are described. The disintegration of carbon grains in interstell

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