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Paper: Solution of the Radiative Transfer Equation in Rotating Atmospheres and in Winds
Volume: 355, Stars With the B[e] Phenomenon
Page: 75
Authors: Korcakova, D.; Kubat, J.
Abstract: We present a method for solving the radiative transfer equation appropriate for its solution in the circumstellar environment of B[e] stars. The problem is solved in two dimensions in axial symmetry. The velocity field in the radiative transfer is included using the Lorentz transformation, which allows us to solve it in the fast polar wind as well as in the slow equatorial wind.
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