A spectral difference between silicates in comet Halley and interstellar silicates.

Details A spectral difference between silicates in comet Halley and interstellar silicates. A spectral difference between silicates in comet Halley and interstellar silicates.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.411c&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 411 - 413

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Interstellar Matter: Silicates, Comets: Silicates, Comet 1986 Iii Halley, Comets: Infrared Spectra

Scientific paper

The authors have obtained an intermediate resolution spectrum of the 8 to 13 μm region in comet Halley which shows a prominent silicate emission feature with structure not observed before in other comets or in interstellar silicates. They confirm the presence of a strong 11.3 μm peak reported by Bregman et al. (1987) and find evidence for additional structure in the band.

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