Processing of Presolar Grains Around Post-AGB Stars: Silicon Carbide as the Carrier of the ``21'' Micron Feature

Details Processing of Presolar Grains Around Post-AGB Stars: Silicon Carbide as the Carrier of the ``21'' Micron Feature Processing of Presolar Grains Around Post-AGB Stars: Silicon Carbide as the Carrier of the ``21'' Micron Feature

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1155s&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1155

Physics

1

Scientific paper

New laboratory data indicate that SiC (cubic or nano crystals) produces
the emission features observed near 21 microns from post-agb stars. The
cold temperature of the dust filters out the main peak. This assignment
lacks the problems associated with previous attributions.

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