M. Curé, I. Araya, C. Arcos, N. Machuca, A. Rodríguez
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Hydrodynamic solutions of radiation driven wind from hot stars
Abstract We show the application of the δ- and Ω-slow hydrodynamical solutions to describe the velocity profiles of massive stars. In particular, these solutions can help to unravel some of the problems within the winds of massive stars such as the approximation of the β-law for the velocity profile of B supergiant stars and the slow outflow wind observed in Be stars.
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