Infrared spectroscopy of interstellar dust

Details Infrared spectroscopy of interstellar dust Infrared spectroscopy of interstellar dust

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987qjras..28..303w&link_type=abstract

Royal Astronomical Society, Quarterly Journal (ISSN 0035-8738), vol. 28, Sept. 1987, p. 303-311.

Astronomy and Astrophysics

Astronomy

13

Astronomical Spectroscopy, Cosmic Dust, Infrared Astronomy, Interstellar Matter, Milky Way Galaxy, Molecular Clouds, Absorption Spectra, Chemical Composition, Galactic Nuclei, Line Of Sight, Optical Thickness

Scientific paper

IR spectroscopy provides a valuable technique for investigating the composition and evolution of interstellar grain material in a variety of astrophysical environments. This paper briefly reviews proposed identifications for the observed features, and discusses some recent observations of the Taurus dark cloud and the Galactic center region. The detection of deep 3-micron absorption towards the Galactic center casts doubt on the assumption that this line of sight is representative of the diffuse interstellar medium.

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