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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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