Diatomic oxide interstellar grains

Details Diatomic oxide interstellar grains Diatomic oxide interstellar grains

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183..177m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, Apr. 1978, p. 177-185. Research supported by the National Research

Astronomy and Astrophysics

Astronomy

20

Diatomic Molecules, Granular Materials, Infrared Absorption, Interstellar Matter, Metal Oxides, Calcium Oxides, Iron Oxides, Magnesium Oxides, Silicates, Silicon Oxides

Scientific paper

The formation of diatomic oxide grains in the interstellar medium is briefly discussed, and the infrared properties of several oxide materials are presented. It is shown that SiO has a broad featureless absorption profile centred at 9.6 microns, while FeO has an absorption peak at 19 microns. A discussion of the wavelength dependence of polarization at 10 microns is also given.

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