Dust formation in stellar winds. IV - Heteromolecular carbon grain formation and growth

Details Dust formation in stellar winds. IV - Heteromolecular carbon grain formation and growth Dust formation in stellar winds. IV - Heteromolecular carbon grain formation and growth

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...206..153g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 206, no. 1, Nov. 1988, p. 153-168.

Astronomy and Astrophysics

Astrophysics

142

Carbon Stars, Cosmic Dust, Interstellar Chemistry, Stellar Envelopes, Stellar Winds, Acetylene, Hydrogen, Nucleation, Reaction Kinetics

Scientific paper

Classical nucleation theory is extended to allow for arbitrary chemical
reactions in the nucleation and growth process. The appropriate
equations describing nucleation and grain growth including chemical
reactions and chemical sputtering are derived and applied to the
formation of carbon grains by reactions with acetylene and hydrogen.

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