Computer Science
Scientific paper
Nov 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990natur.348..293l&link_type=abstract
Nature (ISSN 0028-0836), vol. 348, Nov. 22, 1990, p. 293-298. Research supported by NASA.
Computer Science
101
Carbon Stars, Interstellar Matter, Meteoritic Composition, Meteoroids, Silicon Carbides, Abundance, Asymptotic Giant Branch Stars, Chemical Composition, Cosmic Dust, Interstellar Gas, Stellar Winds
Scientific paper
All five gases in interstellar silicon carbide grains have grossly nonsolar isotopic and elemental abundances that vary with grain size but are strikingly similar to calculated values for the helium-burning shell of low-mass carbon stars. Apparently these grains formed in carbon-star envelopes, and were impregnated with noble gas ions from a stellar wind. Meteoritic SiC provides a detailed record of nuclear and chemical processes in carbon stars.
Amari Sachiko
Anders Edward
Lewis Roy S.
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