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Radiative Transfer in Axial Symmetry

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stellar w<strong>in</strong>d<br />

– optically thick atmospheric regions +<br />

optically th<strong>in</strong> w<strong>in</strong>d<br />

– polar + equatorial region<br />

– static layers + fast outer region<br />

– stellar w<strong>in</strong>d + rotation<br />

– Be, B[e] stars

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