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| Paper: |
Stationary Model of a Line Driven Wind with Rotation |
| Volume: |
388, Mass Loss from Stars and the Evolution of Stellar Clusters |
| Page: |
155 |
| Authors: |
Ceniga, M.; Krticka, J.; Kubát, J. |
| Abstract: |
The theory of radiatively driven wind of Castor, Abbott, and Klein is used for a description of hot star winds. We developed a code using the Newton-Raphson method to get a 1D solution of a line driven isothermal wind. The influence of rotation on the wind solution is studied. |
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