Number of the records: 1  

Influence of the velocity gradient on the line formation in discs of cataclysmic variables

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    SYSNO ASEP0367966
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleInfluence of the velocity gradient on the line formation in discs of cataclysmic variables
    Author(s) Korčáková, Daniela (ASU-R)
    Nagel, T. (DE)
    Werner, K. (DE)
    Suleimanov, V. (RU)
    Votruba, Viktor (ASU-R) RID
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 529, May (2011), A119/1-A119/8
    Number of pages8 s.
    Languageeng - English
    CountryFR - France
    Keywordsradiative transfer ; numerical methods ; cataclysmic variables
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGP205/09/P476 GA ČR - Czech Science Foundation (CSF)
    LC06014 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000289557200127
    DOI10.1051/0004-6361/201015900
    AnnotationWe investigate the influence of the Keplerian velocity gradient on the line formation in CV discs. We show line-profile changes and limb-darkening dependences for the Hα and Hγ lines in a model of SS Cyg, along with the HeI 4923 Å line of a model representing a typical AM CVn system. Both systems are considered in the quiescent phase.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2012
Number of the records: 1  

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