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Compound‐specific Isotope Analysis of the Organic Constituents in Carbonaceous Chondrites by M. A. Sephton; I. Gilmour is a Chemistry article available to read on EtoBox.

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## Abstract | I. | Introduction | 111 | | II. | Stable Isotopes | 112 | | III. | CSIA | 112 | | IV. | CSIA of Organic Compounds from Carbonaceous Chondrites | 115 | | | A. Carbon | 115 | | | B. Nitrogen | 118 | | | C. Sulfur | 118 | | | D. Hydrogen | 118 | | V. | History of Meteoritic Organic Matter | 118 | | Acknowledgments | 118 | | References | 118 | The carbonaceous chondrite meteorites contain evidence of the formation of the solar system, part of which is present within organic matter. In recent years, compound‐specific isotope analysis (CSIA) has been useful in deciphering this complex record. The current published data set provides an insight into the source environments and reaction mechanisms that have contributed to the final state of the organic constituents in carbonaceous chondrites. This review summarises the CSIA data and related key interpretations. © 2001 John Wiley & Sons, Inc., Mass Spec Rev 20:111–120, 2001

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Author
M. A. Sephton; I. Gilmour
Publisher
John Wiley and Sons; Wiley (John Wiley & Sons); John Wiley & Sons Inc.; Wiley (ISSN 0277-7037)
Published
2001
Language
EN
Field
Chemistry (Physical Sciences)

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