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Growth of interstellar grains by coagulation
Authors:S. Simons  I. P. Williams
Affiliation:1. Dept. of Applied Mathematics, Queen Mary College, London, England
Abstract:A discussion is given of the spontaneous coagulation of interstellar grains due to their natural Brownian motion. It is shown that the predicted present day size of such grains, assuming such a mechanism being operative, is in reasonable agreement with observations for three different environments that have been considered: namely, normal interstellar gas clouds, molecular clouds and the atmospheres of cool stars.
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