Low-temperature optical properties of silicate particles in the far-infrared region

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Abstract

The far-infrared absorption spectra of crystalline circumstellar dust analogues (orthoenstatite, clinoenstatite, diopside, and forsterite) were measured at room temperature (295 K) and liquid-helium temperature (4.2 K). The wavelength ranges of the measurements were 20-80 μm and 30-80 μm at 295 K and 4.2 K, respectively. The absorption bands were detected very clearly not only at room temperature, but also at liquid-helium temperature. The temperature effects were clearly observed at liquid-helium temperature, such as (1) an increase in the spectral index of the continuum, (2) an enhancement in the absorption band strength, (3) a decrease in the band width, and (4) the absorption peaks of all bands of all samples shifted toward a shorter wavelength. These results suggest that a reconsideration of the identification should be required for some absorption bands which have been recognized as unidentified bands because of a disagreement in the peak position between the observed data and the laboratory data obtained at room temperature. Our experimental data can be obtained from the web-site (http://www.kyoto-phu.ac.jp/labo/butsuri/).

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Chihara, H., Koike, C., & Tsuchiyama, A. (2001). Low-temperature optical properties of silicate particles in the far-infrared region. Publications of the Astronomical Society of Japan, 53(2), 243–250. https://doi.org/10.1093/pasj/53.2.243

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