Cool Stars with Excesses of Heavy Elements pp 307-312 | Cite as
Dust Formation in Stellar Winds
Conference paper
Abstract
Classical nucleation theory is applied to grain formation in C-rich cool stellar winds of heavily obscured objects. The effectivity of the formation process and its implications for the structure of the shells are discussed.
Keywords
Optical Depth Radiation Pressure Stellar Wind Carbon Star Classical Nucleation Theory
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© D. Reidel Publishing Company, Dordrecht, Holland 1985