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Morlok, A.; Köhler, M. and Grady, M. M.
(2006).
URL: http://www.lpi.usra.edu/meetings/lpsc2006/pdf/1519...
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.