Stationary Model of a Line Driven Wind with Rotation

Details Stationary Model of a Line Driven Wind with Rotation Stationary Model of a Line Driven Wind with Rotation

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..155c&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

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Scientific paper

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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