Time dependent models of grain formation around carbon stars.

Details Time dependent models of grain formation around carbon stars. Time dependent models of grain formation around carbon stars.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339...73e&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 73 - 76

Physics

Carbon Stars: Dust Grains, Carbon Stars: Mass Loss, Carbon Stars: Models

Scientific paper

Carbon-rich asymptotic giant branch stars are sites of dust formation and undergo mass loss at rates ranging from 10-7 to 10-4Msun/yr. The state-of-the-art in modeling these processes is time-dependent models which simultaneously solve the grain formation and gas dynamics problem. The authors present results from such a model, which also includes an exact solution of the radiative transfer within the system.

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