Publication details
Stationary Model of a Line Driven Wind with Rotation
| Authors | |
|---|---|
| Year of publication | 2008 |
| Type | Article in Proceedings |
| Conference | Mass Loss from Stars and the Evolution of Stellar Clusters |
| MU Faculty or unit | |
| Citation | |
| web | http://aspbooks.org/custom/publications/paper/388-0155.html |
| Field | Astronomy and astrophysics |
| Keywords | stellar wind |
| Description | 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. |