Journal
CHEMIE DER ERDE-GEOCHEMISTRY
Volume 65, Issue 2, Pages 93-166Publisher
ELSEVIER GMBH
DOI: 10.1016/j.chemer.2005.01.001
Keywords
presolar grains; interstellar dust; asymptotic giant branch (AGB) stars; novae; supernovae; nucleosynthesis; isotopic ratios; meteorites
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This review provides an introduction to presolar grains - preserved stardust from the interstellar molecular cloud from which our solar system formed - found in primitive meteorites. We describe the search for the presolar components, the currently known presolar mineral populations, and the chemical and isotopic characteristics of the grains and dust-forming stars to identify the grains' most probable stellar sources. (C) 2005 Elsevier GmbH. All rights reserved.
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