Constraints on the thermal history of the Allende (CV3) meteorite by gradual and stepwise pyrolyses of insoluble organic matter
Author:
Affiliation:
1. Department of Earth and Environmental Sciences, Nagoya University
2. Research Institute for Global Change, Japan Agency for Marine-Earth Science and Technology
Publisher
Geochemical Society of Japan
Subject
Geochemistry and Petrology,Geophysics
Link
https://www.jstage.jst.go.jp/article/geochemj/54/4/54_2.0589/_pdf
Reference47 articles.
1. Aléon, J. (2010) Multiple origins of nitrogen isotopic anomalies in meteorites and comets. Astrophys. J. 722, 1342−1351.
2. Aléon, J., Engrand, C., Robert, F. and Chaussidon, M. (2001) Clues to the origin of interplanetary dust particles from the isotopic study of their hydrogen-bearing phases. Geochim. Cosmochim. Acta 65, 4399−4412.
3. Alexander, C. M. O’D., Russell, S. S., Arden, J. W., Ash, R. D., Grady, M. M. and Pillinger, C. T. (1998) The origin of chondritic macromolecular organic matter: A carbon and nitrogen isotope study. Meteorit. Planet. Sci. 33, 603−622.
4. Alexander, C. M. O’D., Fogel, M., Yabuta, H. and Cody, G. D. (2007) The origin and evolution of chondrites recorded in the elemental and isotopic compositions of their macromolecular organic matter. Geochim. Cosmochim. Acta 71, 4380−4403.
5. Alexander, C. M. O’D., Newsome, S. D., Fogel, M. L., Nittler, L. R., Busemann, H. and Cody, G. D. (2010) Deuterium enrichments in chondritic macromolecular material—Implications for the origin and evolution of organics, water and asteroids. Geochim. Cosmochim. Acta 74, 4417−4437.
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