Presolar Graphite from Murchison

Physics

Scientific paper

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Scientific paper

We have analyzed 1642 graphite grains from four Murchison fractions.
Many grains in lower-density fractions KE3 and KFA1 originated from
supernovae. A significant number of grains in higher-density fractions
KFB1 and KFC1 formed in low-metallicity AGB stars.

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