Number of the records: 1  

Z CVn - Still mysterious

  1. 1.
    SYSNO ASEP0500547
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleZ CVn - Still mysterious
    Author(s) Skarka, Marek (ASU-R) ORCID
    Liška, J. (CZ)
    Dřevěný, R. (CZ)
    Sódor, A. (HU)
    Kolenberg, B. (BE)
    Source TitleOpen European Journal on Variable stars. - : Sekce pozorovatelů proměnných hvězd České astronomické společnosti - ISSN 1801-5964
    Roč. 187, March (2018), s. 32-34
    Number of pages3 s.
    ActionConference on Variable Stars Research /49./
    Event date03.11.2017 - 05.11.2017
    VEvent locationBrno
    CountryCZ - Czech Republic
    Event typeEUR
    Languageeng - English
    CountryCZ - Czech Republic
    Keywordslong-term pulsation ; short-term pulsation ; Blazhko effect
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    R&D ProjectsGC17-01752J GA ČR - Czech Science Foundation (CSF)
    Institutional supportASU-R - RVO:67985815
    AnnotationWe comment on short- and long-term pulsation period variations of Z CVn, a classical RR Lyrae star with the Blazhko effect. Z CVn shows cyclic-like O-C diagram that can be interpreted as a consequence of binarity throught the light travel time effect. We show that this hypothesis is false and that the observed long-term period variations must be caused by some effect that is intrinsic to the star. We also show that the Blazhko period is not simply anti-correlated with the long-term period variations as was suggested by previous authors.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2019
Number of the records: 1  

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