Diffusion processes in AP stars and white dwarfs

Details Diffusion processes in AP stars and white dwarfs Diffusion processes in AP stars and white dwarfs

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59..318u&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, Mar.-Apr. 1982, p. 318-325.) Soviet Astronomy, vol. 26, Mar.-Apr. 1982, p. 193-197. Transla

Astronomy and Astrophysics

Astronomy

1

A Stars, Chapman-Enskog Theory, Plasma Diffusion, White Dwarf Stars, Diffusion Theory, Stellar Magnetic Fields

Scientific paper

Diffusion processes in a fully ionized, multicomponent plasma are investigated. Kinetic phenomena due both to ions and to electrons are considered. The kinetic coefficients are calculated in the two-polynomial approximation of the Chapman-Enskog method. The influence of the magnetic field on transport phenomena is taken into account. The results obtained are compared in detail with the results of other authors. In conclusion, possible astrophysical applications of the theory (surface layers of Ap stars and white dwarfs) are briefly discussed.

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