The observational signatures of convectively excited gravity modes in main-sequence stars

@article{Shiode2013TheOS,
  title={The observational signatures of convectively excited gravity modes in main-sequence stars},
  author={Joshua H. Shiode and Eliot Quataert and Matteo Cantiello and Lars Bildsten},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={430},
  pages={1736-1745}
}
We predict the flux and surface velocity perturbations produced by convectively excited gravity modes (g-modes) in main-sequence stars. Core convection in massive stars can excite g-modes to sufficient amplitudes to be detectable with high-precision photometry by Kepler and Convection, Rotation and planetary Transits (CoRoT), if the thickness of the convective overshoot region is 30percent of a pressure scale height. The g-modes manifest as excess photometric variability, with amplitudes of ∼10… Expand

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