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Infrared spectroscopy of circumstellar dust: signs of differentiated materials?

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

Abstract

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
OAI identifier: oai:oro.open.ac.uk:8691
Provided by: Open Research Online

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