The eccentric massive binary V380 Cyg: revised orbital elements and interpretation of the intrinsic variability of the primary component (CROSBI ID 199535)
Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Tkachenko, A. ; Degroote, P. ; Aerts, C. ; Pavlovski, Krešimir ; Southworth, J. ; Papics, P. I. ; Moravveji, E. ; Kolbas, Vladimir ; Tsymbal, V. ; Debosscher, J. ; Clemer, K.
engleski
The eccentric massive binary V380 Cyg: revised orbital elements and interpretation of the intrinsic variability of the primary component
We present a detailed analysis and interpretation of the high-mass binary V380 Cyg, based on high-precision space photometry gathered with the Kepler space mission as well as high-resolution ground-based spectroscopy obtained with the hermes spectrograph attached to the 1.2m Mercator telescope. We derive a precise orbital solution and the full physical properties of the system, including dynamical component mass estimates of 11.43±0.19 and 7.00±0.14 M⊙ for the primary and secondary, respectively. Our frequency analysis reveals the rotation frequency of the primary in both the photometric and spectroscopic data and additional low-amplitude stochastic variability at low frequency in the space photometry with characteristics that are compatible with recent theoretical predictions for gravity-mode os-cillations excited either by the convective core or by sub-surface convective layers. Doppler Imaging analysis of the Silicon lines of the primary suggests the presence of two high-contrast stellar surface abundance spots which are located either at the same latitude or longitude. Comparison of the observed properties of the binary with present-day single-star evolutionary models shows that the latter are inadequate and lack a serious amount of near-core mixing.
binaries; eclipsing binaries; stars; fundamental parameters; oscillations
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Podaci o izdanju
438 (4)
2014.
3093-3110
objavljeno
0035-8711
10.1093/mnras/stt2421