Presolar silicate grains: Abundances, isotopic and elemental compositions, and the effects of secondary processing
Author:
Affiliation:
1. Laboratory for Space Sciences, Washington University
2. Physics Department, Washington University
3. Department of Earth and Planetary Sciences, Washington University
Publisher
Geochemical Society of Japan
Subject
Geochemistry and Petrology,Geophysics
Link
https://www.jstage.jst.go.jp/article/geochemj/50/1/50_2.0377/_pdf
Reference180 articles.
1. Abreu, N. M. and Brearley, A. J. (2010) Early solar system processes recorded in the matrices of two highly pristine CR3 carbonaceous chondrites, MET 00426 and QUE 99177. Geochim. Cosmochim. Acta 74, 1146–1171.
2. Alexander, C. M. O’D., Nittler, L. R. and Tera, F. (2001) The search for presolar silicates and the 54Cr carrier. Lunar Planet. Sci. XXXII, #2191.
3. Amari, S., Anders, E., Virag, A. and Zinner, E. (1990) Interstellar graphite in meteorites. Nature 345, 238–240.
4. Amari, S., Lewis, R. S. and Anders, E. (1994) Interstellar grains in meteorites: I. Isolation of SiC, graphite, and diamond; size distributions of SiC and graphite. Geochim. Cosmochim. Acta 58, 459–470.
5. Anders, E. and Zinner, E. (1993) Interstellar grains in primitive meteorites: diamond, silicon carbide, and graphite. Meteoritics 28, 490–514.
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