Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-09-25
Astronomy and Astrophysics
Astrophysics
8 pages, proceedings of Cool Stars 15, St. Andrews, July 2008, to be published in the Conference Proceedings Series of the Ame
Scientific paper
10.1063/1.3099102
Much effort has been invested in recent years, both observationally and theoretically, to understand the interacting processes taking place in planetary systems consisting of a hot Jupiter orbiting its star within 10 stellar radii. Several independent studies have converged on the same scenario: that a short-period planet can induce activity on the photosphere and upper atmosphere of its host star. The growing body of evidence for such magnetic star-planet interactions includes a diverse array of photometric, spectroscopic and spectropolarimetric studies. The nature of which is modeled to be strongly affected by both the stellar and planetary magnetic fields, possibly influencing the magnetic activity of both bodies, as well as affecting irradiation and non-thermal and dynamical processes. Tidal interactions are responsible for the circularization of the planet orbit, for the synchronization of the planet rotation with the orbital period, and may also synchronize the outer convective envelope of the star with the planet. Studying such star-planet interactions (SPI) aids our understanding of the formation, migration and evolution of hot Jupiters.
Aigrain Suzanne
Cranmer Steven
Fares Rim
Fridlund Malcolm
Pont Frederic
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