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Multicomponent radiatively driven stellar winds. I. Nonisothermal three-component wind of hot B stars

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    0124770 - ASU-R 20010023 RIV FR eng J - Journal Article
    Krtička, Jiří - Kubát, Jiří
    Multicomponent radiatively driven stellar winds. I. Nonisothermal three-component wind of hot B stars.
    Astronomy & Astrophysics. Roč. 369, č. 1 (2001), s. 222-238. ISSN 0004-6361. E-ISSN 1432-0746
    R&D Projects: GA AV ČR KSK1003601; GA AV ČR KSK1043601
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : hydrodynamics * stars mass loss * stars early type * stars winds
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 2.790, year: 2000

    Nonisothermal winds of hot B stars are computed. Friction heats outer parts of the wind and modified temperature stratification ledds to a decrease of the outflow velocity.
    Permanent Link: http://hdl.handle.net/11104/0023029
     

Number of the records: 1  

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