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@inproceedings{872308, author = {Ceniga, Michal and Krtička, Jiří and Kubát, Jiří}, address = {San Francisco, USA}, booktitle = {Mass Loss from Stars and the Evolution of Stellar Clusters}, keywords = {stellar wind}, language = {eng}, location = {San Francisco, USA}, isbn = {978-1-58381-644-8}, pages = {155-156}, publisher = {Astronomical Society of the Pacific}, title = {Stationary Model of a Line Driven Wind with Rotation}, url = {http://aspbooks.org/custom/publications/paper/388-0155.html}, year = {2008} }
TY - JOUR ID - 872308 AU - Ceniga, Michal - Krtička, Jiří - Kubát, Jiří PY - 2008 TI - Stationary Model of a Line Driven Wind with Rotation PB - Astronomical Society of the Pacific CY - San Francisco, USA SN - 9781583816448 KW - stellar wind UR - http://aspbooks.org/custom/publications/paper/388-0155.html N2 - 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. ER -
CENIGA, Michal, Jiří KRTIČKA a Jiří KUBÁT. Stationary Model of a Line Driven Wind with Rotation. In \textit{Mass Loss from Stars and the Evolution of Stellar Clusters}. San Francisco, USA: Astronomical Society of the Pacific, 2008, s.~155-156. ISBN~978-1-58381-644-8.
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