Tytuł artykułu
Autorzy
Wybrane pełne teksty z tego czasopisma
Identyfikatory
Warianty tytułu
Języki publikacji
Abstrakty
We present an extensive analysis of new light and radial velocity (RV) curves, as well as high quality broadening function (BF) profiles of twelve binary systems for which a contact configuration with large temperature differences between components has been reported in the literature. We find that six systems (V1010 Oph, WZ Cyg, VV Cet, DO Cas, FS Lup, V747 Cen) have near contact configurations. For the remaining systems (CX Vir, FT Lup, BV Eri, FO Hya, CN And, BX And), our solutions of the new observations once again converge in a contact configuration with large temperature differences between the components. However, the bright regions discovered in the BFs for V747 Cen, CX Vir, FT Lup, BV Eri, FO Hya, and CN And, and further attributed to hot spots, shed new light on the physical processes taking place between the components and imply the possibility that the contact configurations obtained from light and RV curve modeling are a spurious result.
Słowa kluczowe
binaries: eclipsing
binaries: close
stars: fundamental parameters
stars: individual: V1010 Oph
stars: individual: WZ Cyg
stars: individual: VV Cet
stars: individual: DO Cas
stars: individual: FS Lup
stars: individual: V747 Cen
stars: individual: CX Vir
stars: individual: FT Lup
stars: individual: BV Eri
stars: individual: FO Hya
stars: individual: CN And
stars: individual: BX And
Czasopismo
Rocznik
Tom
Strony
305--336
Opis fizyczny
Bibliogr. 78 poz., rys., tab., wykr.
Twórcy
autor
- Astronomical Observatory of the Jagiellonian University, ul. Orla 171, 30-244 Kraków, Poland
autor
- Astronomical Observatory of the Jagiellonian University, ul. Orla 171, 30-244 Kraków, Poland
autor
- Astronomical Observatory of the Jagiellonian University, ul. Orla 171, 30-244 Kraków, Poland
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-c16e2120-d721-405a-a62e-a476457f3620