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@inproceedings{486930, author = {Krtička, Jiří}, address = {San Francisco, USA}, booktitle = {Stellar Atmosphere Modeling}, keywords = {stars: mass-loss; stars: early-type; hydrodynamics}, language = {eng}, location = {San Francisco, USA}, isbn = {1-58381-131-1}, pages = {259-262}, publisher = {The Astronomical Society of the Pacific}, title = {Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method}, url = {http://arxiv.org/abs/astro-ph/0303030}, year = {2003} }
TY - JOUR ID - 486930 AU - Krtička, Jiří PY - 2003 TI - Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method PB - The Astronomical Society of the Pacific CY - San Francisco, USA SN - 1583811311 KW - stars: mass-loss KW - stars: early-type KW - hydrodynamics UR - http://arxiv.org/abs/astro-ph/0303030 N2 - We present a simple method for the solution of one-component and multicomponent hydrodynamic equations based on the Newton-Raphson method. We show that this method can be used for the solution of stationary hydrodynamic equations. This method has been used for the calculation of the low density stellar wind models for which the multicomponent nature of the wind influences the overall wind structure. ER -
KRTIČKA, Jiří. Modeling of Multicomponent Radiatively Driven Stellar Winds Using a Newton-Raphson Method. In \textit{Stellar Atmosphere Modeling}. San Francisco, USA: The Astronomical Society of the Pacific, 2003, p.~259-262. ISBN~1-58381-131-1.
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