作者: V. I. Shematovich
DOI: 10.1134/S0038094612060068
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摘要: In recent years, a rapid growth in new area of space studies—astrochemistry—has been observed. Its subject is the chemical evolution and diversity interstellar matter. Molecules yield unique information concerning physical conditions medium and, particular, star-formation regions, through spectral observations matter gas-phase dust fractions via rotational vibrational transitions molecules. Moreover, an understanding chemistry molecules can tell us about lifetime history observed objects. Such understanding, however, requires detailed knowledge reactions grain-surface processes that very often take place under rather exotic strongly differing from those for laboratory. Note interests chemists astronomers this are different: more likely to be interested throughout Universe, whereas use as probes processes.