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- W1487685722 abstract "Small inclusions (diameters ranging from 0.001 microns to 10 microns) of isotopically anomalous material within meteorites were almost certainly produced in mass-losing stars. These solid particles preserved their individual identities as they passed through the interstellar medium and the pre-solar nebular. The relationship between studies of meteorites and mass-losing red giants is explored." @default.
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- W1487685722 date "1995-01-01" @default.
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- W1487685722 title "The enrichment of the ISM: Evolved stars and meteorites" @default.
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