Solution of the radiative transfer equation in rotating atmospheres and in winds

被引：0

作者：

Korcakova, Daniela ^{[1
]}

Kubat, Jiri ^{[1
]}

机构：

[1] Acad Sci Czech Republic, Inst Astron, Fricova 298, CZ-25165 Ondrejov, Czech Republic

来源：

STARS WITH THE B[E] PHENOMENON, PROCEEDINGS | 2006年 / 355卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：75 / +

页数：2

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