Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-06-20
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Published in Sience, 19 June 2009, vol. 324, p. 1540
Scientific paper
10.1126/science.1171913
Seismology of stars provides insight into the physical mechanisms taking place in their interior, with modes of oscillation probing different layers. Low-amplitude acoustic oscillations excited by turbulent convection were detected four decades ago in the Sun and more recently in low-mass main-sequence stars. Using data gathered by the Convection Rotation and Planetary Transits mission, we report here on the detection of solar-like oscillations in a massive star, V1449 Aql, which is a known large-amplitude (b Cephei) pulsator.
Appourchaux Thierry
Auvergne Michel
Baglin Annie
Baudin Francois
Belkacem Kevin
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