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Infrared spectroscopy of circumstellar dust: signs of differentiated materials?

By A. Morlok, M. Köhler and M. M. Grady


Mid-infrared absorption spectra of powdered achondrites are compared with the astronomical spectra of dust around young, evolving stars, to find evidence (or not) of dust formed in collisional cascades of material from planetesimals

Year: 2006
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Provided by: Open Research Online

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