A hidden reservoir of Fe/FeS in interstellar silicates?
M. K\"ohler, A. Jones, N. Ysard

TL;DR
This study investigates the incorporation of iron and sulphur into interstellar amorphous silicates, revealing that Fe/FeS nano-inclusions can be embedded without significantly altering observable spectral features, thus explaining their elusive nature in space.
Contribution
It introduces a model for Fe and S incorporation into amorphous silicates using effective-medium theory, matching observed interstellar silicate features and suggesting hidden reservoirs of Fe/FeS.
Findings
Fe/FeS nano-inclusions do not significantly alter optical properties.
A mixture of olivine- and pyroxene-type silicates broadens spectral features.
Amorphous carbon mantles increase short-wavelength absorption.
Abstract
The depletion of iron and sulphur into dust in the interstellar medium and the exact nature of interstellar amorphous silicate grains is still an open question. We study the incorporation of iron and sulphur into amorphous silicates of olivine- and pyroxene-type and their effects on the dust spectroscopy and thermal emission. We used the Maxwell-Garnett effective-medium theory to construct the optical constants for a mixture of silicates, metallic iron, and iron sulphide. We also studied the effects of iron and iron sulphide in aggregate grains. Iron sulphide inclusions within amorphous silicates that contain iron metal inclusions shows no strong differences in the optical properties of the grains. A mix of amorphous olivine- and pyroxene-type silicate broadens the silicate features. An amorphous carbon mantle with a thickness of 10 nm on the silicate grains leads to an increase in…
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