Calculations of infrared fluxes from galactic sources for a polysaccharide grain model

Details Calculations of infrared fluxes from galactic sources for a polysaccharide grain model Calculations of infrared fluxes from galactic sources for a polysaccharide grain model

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..53..489h&link_type=abstract

Astrophysics and Space Science, vol. 53, no. 2, Feb. 1978, p. 489-505.

Astronomy and Astrophysics

Astronomy

8

Astronomical Models, Cosmic Dust, Galactic Radiation, Infrared Astronomy, Polysaccharides, Molecular Spectra, O Stars, Opacity, Optical Thickness, Stellar Mass Ejection, Transmittance

Scientific paper

Transmittance data appropriate for grain material which is predominantly comprised of polysaccharides are used to compute infrared fluxes from several types of galactic infrared source. The model used in these computations involves polysaccharide condensation in material flowing out from O-type stars. With the exception of rather minor discrepancies it is shown that it is possible to match the 2.1-13-micron observations of a wide range of galactic infrared sources.

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