Radiative Transfer in Axial Symmetry
Radiative Transfer in Axial Symmetry
Radiative Transfer in Axial Symmetry
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Where it can play the role?<br />
– edge-on view – open<strong>in</strong>g angle ∼ 10 ◦<br />
– not so small probability<br />
– self-shield<strong>in</strong>g disc (e.g. V348 Pup)<br />
– occult<strong>in</strong>g systems – some UX UMa or SW Ser<br />
systems<br />
– low lum<strong>in</strong>osity<br />
– dust is not important <strong>in</strong> most CVs (<strong>in</strong> contrast to<br />
polars)<br />
– extended area<br />
– w<strong>in</strong>d<br />
– important corona – polars, <strong>in</strong>termediate polars
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