Atmospheres and Winds of M- and C-type AGB stars

Details Atmospheres and Winds of M- and C-type AGB stars Atmospheres and Winds of M- and C-type AGB stars

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..872h&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

Computer Science

3

Giant And Subgiant Stars, Low Luminosity Stars, Subdwarfs, And Brown Dwarfs, Mass Loss And Stellar Winds

Scientific paper

Mass loss of asymptotic giant branch (AGB) stars is commonly attributed to the combined effects of pulsation-induced shocks and radiation pressure on dust grains formed in the outer atmospheric layers. This paper discusses recent results of detailed radiation-hydrodynamical wind models, regarding the composition of silicate grains in M-type AGB stars, the influence of grain size dependent opacities, and basic differences in dust-driven outflows of C- and M-type AGB stars.

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