The plausibility of silicate-core ice-mantle grains

Details The plausibility of silicate-core ice-mantle grains The plausibility of silicate-core ice-mantle grains

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..34..185d&link_type=abstract

(Symposium on Solid State Astrophysics, Cardiff, Wales, July 9-12, 1974.) Astrophysics and Space Science, vol. 34, Apr. 1975, p.

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Infrared Astronomy, Interstellar Extinction, Interstellar Matter, Light Curve, Silicates, Absorption Spectra, Astronomical Models, Ice, Optical Polarization

Scientific paper

Extinction curves for silicate-core ice-mantle grains are computed and compared with the infrared spectral data on the BN object on the Orion nebula. A ratio of outer mantle to core radius of 1.3 which best fits this data suggests that silicate-core ice-mantle grains are unlikely to contribute a major part to the total visual extinction coefficient of interstellar material.

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