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Two-component stellar wind in hot stars

  1. 1.
    0124681 - ASU-R 20000137 RIV US eng C - Conference Paper (international conference)
    Krtička, Jiří - Kubát, Jiří
    Two-component stellar wind in hot stars.
    Thermal and ionization aspects of flows from hot stars: observation and theory. San Francisco: Astronomical society of the Pacific, 2000 - (Lamers, H.; Sapar, A.), s. 235-236. Conference series., 204.
    [Thermal and ionization aspects of flows from hot stars. Tartu (EE), 23.08.1999-27.08.1999]
    R&D Projects: GA AV ČR IAA3003805
    Institutional research plan: CEZ:AV0Z1003909
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    We present the solution of hydrodynamic equations of radiatively driven stellar wind with inclusion of the frictional force. Hydrodynamic equations are solved for absorbing ions and for a passive plasma. We discuss the critical point condition for such wind. We show that friction does not lead not to separation of the two components of the wind of hot stars.
    Permanent Link: http://hdl.handle.net/11104/0022940
     

Number of the records: 1  

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