Transport of dust particles in a protoplanetary accretion disk

Details Transport of dust particles in a protoplanetary accretion disk Transport of dust particles in a protoplanetary accretion disk

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990avest..24..134g&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 24, Apr.-June 1990, p. 134-139. In Russian.

Astronomy and Astrophysics

Astronomy

Accretion Disks, Interplanetary Dust, Protoplanets, Transport Properties, Boltzmann Transport Equation, Molecular Clouds, Organic Compounds, Temperature Effects

Scientific paper

A theory of dust-particle transport through a protoplanetary accretion disk is developed. Arguments are presented in support of the conservation of an organic mantle covering certain particles in molecular clouds, in the accretion process on the disk as well as in the disk itself. It is concluded that particles with an organic mantle of interstellar origin could have formed part of the composition of cometary nuclei.

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