Statistical approach to the theory of circumstellar discs

Details Statistical approach to the theory of circumstellar discs Statistical approach to the theory of circumstellar discs

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.164..231h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 164, no. 2, Feb. 1990, p. 231-256.

Statistics

Computation

5

Computational Astrophysics, Cosmic Dust, Gravitational Fields, Statistical Analysis, Stellar Envelopes, Equations Of Motion, Navier-Stokes Equation, Numerical Integration, Particle Collisions, Particle Emission

Scientific paper

The equations for the viscous motion of a mixture of gas and dust in a gravitational field are derived from the statistics of particle orbits and radiative processes in a general form which gives the Navier-Stokes equation as a special case. Diffusion, partially elastic collisions and - for larger bodies - the gravitational encounters are included. The results are applied to the evolution of circumstellar disks.

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