Constraints on Grain Formation Around Carbon Stars from Laboratory Studies of Presolar Graphite

Details Constraints on Grain Formation Around Carbon Stars from Laboratory Studies of Presolar Graphite Constraints on Grain Formation Around Carbon Stars from Laboratory Studies of Presolar Graphite

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1509b&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1509

Physics

Scientific paper

Realistic models of mass outflows from AGB stars (1.1-5 solar masses)
show that graphite grains grow over a 2-10 y time interval at radii of
2.3-3.7 A.U. Pressure constraints require that grains form in clumps or
jets with enhanced density.

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