Sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars

@article{Reeth2018SensitivityOG,
  title={Sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars},
  author={T. V. Reeth and J. Mombarg and S. Mathis and A. Tkachenko and J. Fuller and D. M. Bowman and B. Buysschaert and C. Johnston and A. G. Hern'andez and J. Goldstein and R. Townsend and C. Aerts},
  journal={Astronomy and Astrophysics},
  year={2018},
  volume={618},
  pages={1-14}
}
  • T. V. Reeth, J. Mombarg, +9 authors C. Aerts
  • Published 2018
  • Physics
  • Astronomy and Astrophysics
  • Context. While rotation has a major impact on stellar structure and evolution, its effects are not well understood. Thanks to high-quality and long-time base photometric observations obtained with recent space missions, we are now able to study stellar rotation more precisely. Aims. We aim to constrain radial differential rotation profiles in γ Doradus (γ Dor) stars, and to develop new theoretical seismic diagnosis for such stars with rapid and potentially non-uniform rotation. Methods… CONTINUE READING
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