The Rise of ROME. I. A Multiwavelength Analysis of the Star-Planet Interaction in the HD 189733 System

@article{Route2019TheRO,
  title={The Rise of ROME. I. A Multiwavelength Analysis of the Star-Planet Interaction in the HD 189733 System},
  author={M. Route},
  journal={The Astrophysical Journal},
  year={2019},
  volume={872},
  pages={79}
}
  • M. Route
  • Published 2019
  • Physics
  • The Astrophysical Journal
  • Several "hot Jupiter" host stars appear to exhibit enhanced chromospheric activity, coronal flaring, and starspot development synchronized to their planetary orbits. These effects have been attributed to tidal and/or magnetic interactions between the star and exoplanet. The best studied among such systems is HD 189733, which has previously been observed from radio to X-ray wavelengths. Here, I present ~4.75 GHz Arecibo radio telescope observations of HD 189733 during a fraction of the exoplanet… CONTINUE READING
    5 Citations

    Figures and Tables from this paper.

    References

    SHOWING 1-10 OF 72 REFERENCES
    FUV VARIABILITY OF HD 189733. IS THE STAR ACCRETING MATERIAL FROM ITS HOT JUPITER
    • 37
    • Highly Influential
    • PDF
    THE CORONA OF HD 189733 AND ITS X-RAY ACTIVITY
    • 41
    • Highly Influential
    • PDF
    Spectropolarimetric observations of the transiting planetary system of the K dwarf HD 189733
    • 85
    • Highly Influential
    • PDF
    MOST space-based photometry of the transiting exoplanet system HD 189733: precise timing measurements for transits across an active star
    • 41
    • Highly Influential
    • PDF
    Stellar activity of planetary host star HD 189 733
    • 118
    • Highly Influential
    • PDF
    Searching for star–planet interactions within the magnetosphere of HD 189733
    • 127
    • PDF