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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, s.~259-262. ISBN~1-58381-131-1.
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