1. Detection of gravity modes in the massive binary V380 Cyg from Kepler space-based photometry and high-resolution spectroscopy
- Author
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Tkachenko, A., Aerts, C., Pavlovski, K., Southworth, J., Degroote, P., Debosscher, J., Still, M., Bryson, S., Molenberghs, G., Bloemen, S., de Vries, B. L., Hrudkova, M., Lombaert, R., Neyskens, P., Papics, P. I., Raskin, G., Van Winckel, H., Morris, R. L., Sanderfer, D. T., and Seader, S. E.
- Subjects
oscillations [stars] ,eclipsing binaries ,binaries: eclipsing – stars: fundamental parameters – stars: individual: V380 Cyg – stars: oscillations – stars: variables: general ,fundamental parameters [stars] ,light curves ,binaries: eclipsing ,stars: fundamental parameters ,stars: individual: V380 Cyg ,stars: oscillations ,stars: variables: general ,FOS: Physical sciences ,asteroseismology ,Astrophysics - Solar and Stellar Astrophysics ,eclipsing [binaries] ,star ,variables: general [stars] ,component ,evolution ,Astrophysics::Solar and Stellar Astrophysics ,individual: v380 cyg [stars] ,Astrophysics::Earth and Planetary Astrophysics ,pulsations ,Solar and Stellar Astrophysics (astro-ph.SR) - Abstract
We report the discovery of low-amplitude gravity-mode oscillations in the massive binary star V380 Cyg, from 180 d of Kepler custom-aperture space photometry and 5 months of high-resolution high signal-to-noise spectroscopy. The new data are of unprecedented quality and allowed to improve the orbital and fundamental parameters for this binary. The orbital solution was subtracted from the photometric data and led to the detection of periodic intrinsic variability with frequencies of which some are multiples of the orbital frequency and others are not. Spectral disentangling allowed the detection of line-profile variability in the primary. With our discovery of intrinsic variability interpreted as gravity mode oscillations, V380 Cyg becomes an important laboratory for future seismic tuning of the near-core physics in massive B-type stars., Comment: 5 pages, 4 figures, 2 tables. Accepted for publication in MNRAS Letters
- Published
- 2012