ROME (Radio Observations of Magnetized Exoplanets). II. HD 189733 Does Not Accrete Significant Material from Its Exoplanet Like a T Tauri Star from a Disk

@article{Route2019ROMEO,
  title={ROME (Radio Observations of Magnetized Exoplanets). II. HD 189733 Does Not Accrete Significant Material from Its Exoplanet Like a T Tauri Star from a Disk},
  author={Matthew Route and Leslie W. Looney},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2019}
}
  • M. Route, Leslie W. Looney
  • Published 2019
  • Physics
  • arXiv: Solar and Stellar Astrophysics
It has been asserted that the primary star in the HD 189733 system steadily accretes evaporated exospheric gases from its ``hot Jupiter'' companion, rather like a T Tauri star accreting from a disk. We conduct statistical and periodogram analyses of the photometric time series of the primary, as acquired by the automated photoelectric telescope (APT), Microvariability and Oscillations of Stars (MOST), and Wise Observatory, to investigate this claim with the goal of revealing the presence of… Expand

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References

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