Number of the records: 1  

Properties and nature of Be stars. 26. Long-term and orbital changes of zetaTauri

  1. 1.
    SYSNO ASEP0338396
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleProperties and nature of Be stars. 26. Long-term and orbital changes of zetaTauri
    Author(s) Ruždjak, D. (HR)
    Božić, H. (HR)
    Harmanec, P. (CZ)
    Fiřt, R. (DE)
    Chadima, P. (CZ)
    Bjorkman, K.S. (US)
    Gies, D. R. (US)
    Kaye, A.B. (US)
    Koubský, Pavel (ASU-R) RID, ORCID
    McDavid, D. (US)
    Richardson, N. (US)
    Sudar, D. (HR)
    Šlechta, Miroslav (ASU-R) RID, ORCID
    Wolf, M. (CZ)
    Yang, S. (CA)
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 506, č. 3 (2009), s. 1319-1333
    Number of pages15 s.
    Languageeng - English
    CountryFR - France
    Keywordsearly-type stars ; spectroscopic ; emission-line
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    R&D ProjectsGA205/03/0788 GA ČR - Czech Science Foundation (CSF)
    GD205/08/H005 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000271514900024
    DOI10.1051/0004-6361/200810526
    AnnotationOur goal is to find the true timescales of its variability and confront them with the existing models related to various aspects of the Be phenomenon.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2010
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.