Can we improve upon astronomical silicate?

Details Can we improve upon astronomical silicate? Can we improve upon astronomical silicate?

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...442..172k&link_type=abstract

The Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 442, no. 1, p. 172-176

Astronomy and Astrophysics

Astrophysics

25

Constraints, Cosmic Dust, Interstellar Extinction, Interstellar Matter, Polarization (Waves), Refractivity, Silicates, Ultraviolet Radiation, Albedo, Grain Size, Mass Distribution, Scattering, Size Distribution

Scientific paper

The refractive indices for 'astronomical silicate' (Draine & Lee)
are widely used for a component of interstellar dust. We report on a
problem which arises when these are used to explain the wavelength
dependence of ultraviolet interstellar polarization, and on a potential
resolution.

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