Journal
ANALYTICAL CHEMISTRY
Volume 85, Issue 3, Pages 1264-1270Publisher
AMER CHEMICAL SOC
DOI: 10.1021/ac303052p
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Tiny dust grains extracted from primitive meteorites are identified to have originated in the atmospheres of stars on the basis of their anomalous isotopic compositions. Although isotopic analysis with the ion microprobe plays a major role in the laboratory analysis of these stardust grains, many other microanalytical techniques are applied to extract the maximum amount of information.
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