On grain-size-dependent chemical fractionation in the early proto-solar cloud

Details On grain-size-dependent chemical fractionation in the early proto-solar cloud On grain-size-dependent chemical fractionation in the early proto-solar cloud

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.147..329a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 147, no. 2, Aug. 1988, p. 329-334.

Astronomy and Astrophysics

Astrophysics

Chemical Fractionation, Cosmochemistry, Grain Size, Interstellar Matter, Protostars, Stellar Evolution, Condensing, Evaporation, Sublimation, Turbulent Diffusion

Scientific paper

The work of Morfill and Volk (1984) on minerals in a turbulent protosolar disk is extended to the case of a variable grain size resulting from the evaporation and recondensation of mineral constituents. Iterations towards a self-consistent solution using numerical integrations reveal that the grains do not grow large enough to significantly affect the coupling between transport and recondensation. The use of new analytical functions allows solutions to be obtained faster than previously.

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