Number of the records: 1  

Time-dependent spectral-feature variations of stars displaying the B[e] phenomenon III. HD 50138

  1. 1.
    SYSNO ASEP0461424
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleTime-dependent spectral-feature variations of stars displaying the B[e] phenomenon III. HD 50138
    Author(s) Jeřábková, T. (CZ)
    Korčáková, D. (CZ)
    Miroshnichenko, A. S. (US)
    Danford, S. (US)
    Zharikov, S.V. (MX)
    Křiček, R. (CZ)
    Zasche, P. (CZ)
    Votruba, Viktor (ASU-R) RID
    Šlechta, Miroslav (ASU-R) RID, ORCID
    Škoda, Petr (ASU-R) RID, ORCID
    Janík, J. (CZ)
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 586, February (2016), A116/1-A116/29
    Number of pages29 s.
    Publication formOnline - E
    Languageeng - English
    CountryFR - France
    KeywordsBe stars ; circumstellar matter ; emission-line
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    Institutional supportASU-R - RVO:67985815
    UT WOS000369715900127
    EID SCOPUS84957605059
    DOI10.1051/0004-6361/201526290
    AnnotationWe describe the spectral variability of HD 50138 over the last twenty years. Based on these data, we determine new restrictions for future modelling. We confirm the quasi-periodic behaviour of the object's spectral variability, which probably reflects mass transfer in a binary system. This behaviour also supports a recently introduced explanation of the nature of FS CMa stars as post-merger systems.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2017
Number of the records: 1  

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