Solution of the Radiative Transfer Equation in Rotating Atmospheres and in Winds

Details Solution of the Radiative Transfer Equation in Rotating Atmospheres and in Winds Solution of the Radiative Transfer Equation in Rotating Atmospheres and in Winds

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..355...75k&link_type=abstract

Stars with the B[e] Phenomenon. ASP Conference Series, Vol. 355, Proceedings of the Conference Held 10-16 July, 2005, at the Isl

Astronomy and Astrophysics

Astronomy

Scientific paper

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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