On the moment method for radiative transfer in spherical dust shells with a core

Details On the moment method for radiative transfer in spherical dust shells with a core On the moment method for radiative transfer in spherical dust shells with a core

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..67...99w&link_type=abstract

Astrophysics and Space Science, vol. 67, no. 1, Jan. 1980, p. 99-103.

Astronomy and Astrophysics

Astrophysics

5

Cosmic Dust, Nongray Gas, Radiation Distribution, Radiative Transfer, Stellar Atmospheres, Boundary Value Problems, Cores, Eddington Approximation, Optical Thickness, Spheres

Scientific paper

A two-shell moment method with three stream division of the radiation field has been suggested for solving radiative transfer problems in a nongray extended dust shell surrounding a central star. The results computed are found to be of comparable accuracy with those of Unno and Kondo, obtained by generalized Eddington approximation. A more simplified approximation has been put forward for an optically thin medium.

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