Number of the records: 1  

Young solar type active stars: the TYC 2627-638-1 system

  1. 1.
    SYSNO ASEP0354860
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleYoung solar type active stars: the TYC 2627-638-1 system
    Author(s) Oláh, K. (HU)
    Korhonen, H. (DE)
    Vida, K. (HU)
    Ilyin, I.V. (DE)
    Dall, T.H. (DE)
    Jarvinen, S.P. (DE)
    Jurcsik, J. (HU)
    Andersen, M.I. (DE)
    Djupvik, A.A. (ES)
    Pursimo, T. (ES)
    Moór, A. (HU)
    Datson, J. (ES)
    Karjalainen, R. (ES)
    Liimets, T. (ES) ORCID
    Kubát, Jiří (ASU-R) RID, ORCID
    Kawka, Adela (ASU-R) ORCID, RID
    Source TitleAstronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
    Roč. 515, June (2010), A81/1-A81/11
    Number of pages11 s.
    Languageeng - English
    CountryFR - France
    Keywordsstars ; activity ; atmospheres
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    CEZAV0Z10030501 - ASU-R (2005-2011)
    UT WOS000280505000050
    DOI10.1051/0004-6361/200912892
    AnnotationWe present BV(RI)(C) and JHKs photometry and low-and high-resolution spectroscopy of the 11th mag G-type star TYC 2627-638-1. Our investigation reveals that the target is separated into two young, early-G-type main-sequence (or late pre-main-sequence) stars, which are most probably bound and form a wide binary system. A substellar body orbits the brighter component as implied by radial velocity variations. The brighter component possibly also has a faint, later type stellar companion.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2011
Number of the records: 1  

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