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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Wńodzimierz Bielecki,Dariusz Burakis on determination of the density and temperature structure as well as the velocity field in these objects. The presence of large scale temperature gradients is expected when looking towards embedded heating sources; the frequency with which the expected effects are seen in molecular line data give

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Phoolendra K. Mishra,Kristopher L. Kuhlmanon towards nearby hot stars, the question of molecule formation has accompanied the observational efforts. These early discoveries by Adams, Dunham, Swings, Rosenfeld and McKellar are separated by a gap of 28 years from the radio-discovery of the first polyatomic molecule ( ammonia, NH. ) in interstellar space by Townes and collaborators.

BRACE

Pradipta Banerji,Sanjay Chikermanee far-infrared rotational lines of CO, OH, NH. and HD, together with a brief description of the analysis and interpretation of the spectra, The “state of the art” in instrument performance and the prospects for improved sensitivity and resolution are also surveyed.

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Conference proceedings 1984troscopy of extragalactic sources. The potential of the field in the next decade or two is clear. The lRAS mission has completed one of the pre-requisites, namely an all-sky photometric survey. Major space missions utilising cryogenic infrared telescopes have been approved in Europe (ISO) and seem l

FISC

Absorption and Emission Characteristics of Interstellar Duststressed, 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. Krätschmer and Huffman, 1979, Knacke and Krätschmer, 1980, Day, 1979, Borghesi et al., 1983 and references the

Agronomy

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