Isotopic compositions of C, N, O, Mg, and Si, trace element abundances, and morphologies of single circumstellar graphite grains in four density fractions from the Murchison meteorite
- 31 October 1995
- journal article
- Published by Elsevier in Geochimica et Cosmochimica Acta
- Vol. 59 (19) , 4029-4056
- https://doi.org/10.1016/0016-7037(95)00280-d
Abstract
No abstract availableKeywords
This publication has 85 references indexed in Scilit:
- Interstellar grains in meteorites: III. Graphite and its noble gasesGeochimica et Cosmochimica Acta, 1995
- Interstellar grains in meteorites: I. Isolation of SiC, graphite and diamond; size distributions of SiC and graphiteGeochimica et Cosmochimica Acta, 1994
- The isotopic compositions and stellar sources of meteoritic graphite grainsNature, 1993
- Interstellar Grains in Primitive Meteorites: Diamond, Silicon Carbide, and GraphiteMeteoritics, 1993
- Presolar SiC in chondrites: How variable and how many sources?Geochimica et Cosmochimica Acta, 1993
- Interstellar SiC with unusual isotopic compositions - Grains from a supernova?The Astrophysical Journal, 1992
- Interstellar graphite in meteoritesNature, 1990
- Instabilities and nonradial motion in SN 1987AThe Astrophysical Journal, 1989
- Hydrostatic nucleosynthesis. I - Core helium and carbon burning.The Astrophysical Journal, 1985
- N-14/N-15 isotope fractionation in the reaction N2H/+/ + N2 - Interstellar significanceThe Astrophysical Journal, 1981