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Modelling of resonance lines in ingomogeneous hot star winds

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    0424777 - ASÚ 2014 RS eng J - Journal Article
    Šurlan, Brankica - Hamann, W.-R. - Kubát, Jiří - Oskinova, L.M. - Feldmeier, A.
    Modelling of resonance lines in ingomogeneous hot star winds.
    Publications of the Astronomical Observatory of Belgrade. -, č. 92 (2013), s. 197-200. ISSN 0373-3742.
    [Future science with metre-class telescopes. Beograd, 18.09.2012-21.09.2012]
    R&D Projects: GA ČR GA205/08/0003
    Institutional support: RVO:67985815
    Keywords : stars winds * outflows stars * mass-loss stars
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    We show how different model parameters influence resonance line formation. By modelling ultraviolet resonance lines, we demonstrate how wind inhomogeneities influence line profiles.
    Permanent Link: http://hdl.handle.net/11104/0230794

     
     
Number of the records: 1  

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