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Hydrated Silicates on M-, S-, and E-Type Asteroids as Possible Traces of Collisions with Bodies from the Jupiter Growth Zone
V. V. BusarevVolume:
36
Language:
english
Pages:
8
DOI:
10.1023/a:1014221510387
Date:
January, 2002
File:
PDF, 60 KB
english, 2002