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Modeling of multicomponent radiatively driven stellar winds using a Newton-Raphson method

  1. 1.
    0125261 - ASU-R 20030167 RIV US eng C - Conference Paper (international conference)
    Krtička, Jiří
    Modeling of multicomponent radiatively driven stellar winds using a Newton-Raphson method.
    Stellar atmosphere modeling. San Francisco: Astronomical Society of Pacific, 2003 - (Hubený, I.; Mihalas, D.; Werner, K.), s. 259-262. ASP Conference Series., 288.
    [Stellar Atmosphere Modeling. Tubingen (DE), 08.04.2002-12.04.2002]
    R&D Projects: GA ČR GA205/01/0656; GA ČR GA205/02/0445; GA AV ČR KSK2043105
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : hydrodynamic * equations * Newton-Raphson method
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    The author presents a simple method for the solution of one-component and multicomponent hydrodynamic equations based on the Newton-Raphson method. He showsthat this method can be used for the solution of stationary hydrodynamic equations.
    Permanent Link: http://hdl.handle.net/11104/0023518
     

Number of the records: 1  

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