Abstract
Gürtleret al. (1981) argue that SiO could not be the material responsible for the interstellar 10 micron feature as had been proposed by Duleyet al. (1979). While Millar (1982) has quite successfully refuted the arguments of Gürtleret al. (1981), we present here some additional considerations which indicate that the model of Duleyet al. (1979) requires appreciable modification to be consistent with recent experimental results.
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Nuth, J.A., Donn, B. A note on the composition and structure of interstellar grains. Astrophys Space Sci 95, 175–178 (1983). https://doi.org/10.1007/BF00661168
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DOI: https://doi.org/10.1007/BF00661168