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The enrichment of the ISM: Evolved stars and meteoritesSmall 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.
Document ID
19960003663
Document Type
Conference Paper
Authors
Jura, M. (California Univ. Los Angeles, CA, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1995
Publication Information
Publication: Astronomical Society of the Pacific, Airborne Astronomy Symposium on the Galactic Ecosystem: From Gas to Stars to Dust, Volume 73
Subject Category
Astrophysics
Accession Number
96N13673
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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