Solar-like oscillations in a massive star

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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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.

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