Solution of the comoving-frame equation of transfer in spherically symmetric flows. VII - Angle-dependent partial redistribution

Astronomy and Astrophysics – Astrophysics

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Line Spectra, Radiative Transfer, Stellar Atmospheres, Nebulae, Scattering, Stellar Winds

Scientific paper

A method is presented for treating line scattering with general redistribution in angle and frequency in spherical expanding flows. The scheme employs a solution of the moment equations for the source function coupled with a ray-by-ray formal solution for angular shape factors. In both steps the differencing is straightforward and numerically stable.

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