Meteoritic silicon carbide and its stellar sources - Implications for galactic chemical evolution

Computer Science

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Chemical Evolution, Chondrites, Galactic Evolution, Interstellar Matter, Red Giant Stars, Silicon Carbides, Carbon Isotopes, Carbon Stars, Chemical Composition, Novae, Solar System, Meteorites, Silicon Carbide, Origin, Source, Chemistry, Shock Effects, Evolution, Samples, Meteorite, Carbonaceous Chondrites, Grains, Carbon, Depletion, Isotopes, Abundance, Procedure, Murchison, Laboratory Studies, Heating

Scientific paper

Interstellar silicon carbide grains in meteorites provide a novel means for studying the carbon-star population of about 5 x 10 to the 9th years ago. Their C-12/C-13 ratios differ greatly from the solar value but resemble those of present-day csrbon stars, implying little change in the galactic C-13 inventory. Isotope data on nitrogen and silicon suggest that the silicon carbide grains come mainly from red giants, with small contributions from novae.

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