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Radiation induced coronal wind in late B stars

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    0125241 - ASU-R 20030147 RIV NL eng J - Journal Article
    Kubát, Jiří - Krtička, Jiří - Pustylnik, I. B.
    Radiation induced coronal wind in late B stars.
    New Astronomy. Roč. 9, č. 3 (2004), s. 215-224. ISSN 1384-1076. E-ISSN 1384-1092
    R&D Projects: GA ČR GA205/01/0656; GA ČR GA205/02/0445; GA AV ČR KSK2043105
    Institutional research plan: CEZ:AV0Z1003909
    Keywords : early type stars * coronae stars * hydrodynamics
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
    Impact factor: 2.171, year: 2004

    Multicomponent radiatively driven winds in the late B stars cause significant heating of the layers just above the photosphere. These heated layers form a hot region - a corona, which may provide a significant fraction of energy necessary for the formation of a coronal wind driven by gas pressure.

    Permanent Link: http://hdl.handle.net/11104/0023498

     
     

Number of the records: 1  

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