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Paper: Two-component Stellar Wind in Hot Stars
Volume: 204, Thermal and Ionization Aspects of Flows from Hot Stars: Observations and Theory
Page: 235
Authors: Krtička, J.; Kubát, J.
Abstract: We present results of the solution of hydrodynamic equations of a two-component radiatively driven stellar wind with inclusion of the frictional force. We found that friction does not lead to significant separation of the components. However, the outflow velocity is substantially decreased with respect to the one component model.
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