The size distribution of dust particles in a dust-driven wind

Details The size distribution of dust particles in a dust-driven wind The size distribution of dust particles in a dust-driven wind

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223..227d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 227-236.

Statistics

Computation

53

Computational Astrophysics, Cool Stars, Cosmic Dust, Particle Size Distribution, Stellar Winds, Coagulation, Distribution Functions, Giant Stars, Stellar Envelopes, Stellar Models, Supergiant Stars

Scientific paper

A simple method for the calculation of the particle size spectrum in dust forming objects is presented. The application to a dust driven wind model around a C-star shows a power law size distribution over several orders of magnitude in size. The spectral index is found. Drift velocity between dust and gas leads to a slightly smaller spectral index, while coagulation practically has no influence on the produced size distribution.

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