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Time Dependent Models of Grain Formation Around Carbon Stars (1996)

Egan, M. P. ; Shipman, R. F.

In: CASI

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Publication Date: 2004-12-03

Description: Carbon-rich Asymptotic Giant Branch stars are sites of dust formation and undergo mass loss at rates ranging from 10(exp -7) to 10(exp -4) solar mass/yr. The state-of-the-art in modeling these processes is time-dependent models which simultaneously solve the grain formation and gas dynamics problem. We present results from such a model, which also includes an exact solution of the radiative transfer within the system.

Keywords: Astronomy

Type: From Stardust to Planetesimals: Contributed Papers; 73-76; NASA-CP-3343

Format: text

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