Spectropolarimetry of hot Jupiter systems

R. Fares, J. F. Donati, C. Moutou, Evgenya Shkolnik, D. Bohlender

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

In the past 15 years, tens of giant planets orbiting close to their stars (hot Jupiters) have been discovered - many of them are so close to their host stars (a<0.1 AU) that interactions between the star and the planet are expected (and observed) to occur. Studying these interactions helps understanding the formation, evolution and migration of hot Jupiters. Using spectropolarimetry, we can reconstruct the large-scale magnetic topologies of hot-Jupiter hosting stars and thus quantitatively study such interactions. We present here the results we have obtained on three hot Jupiter systems, having different stellar and planetary parameters.

Original languageEnglish (US)
Title of host publicationAIP Conference Proceedings
Pages437-440
Number of pages4
Volume1094
DOIs
StatePublished - 2009
Externally publishedYes
Event15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom
Duration: Jul 21 2008Jul 25 2008

Other

Other15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
CountryUnited Kingdom
CitySt. Andrews
Period7/21/087/25/08

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Keywords

  • Activity
  • Magnetic fields
  • Planetary systems

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Fares, R., Donati, J. F., Moutou, C., Shkolnik, E., & Bohlender, D. (2009). Spectropolarimetry of hot Jupiter systems. In AIP Conference Proceedings (Vol. 1094, pp. 437-440) https://doi.org/10.1063/1.3099141